579:), with recent studies suggesting a narrower range of 2.5 and 3 kpc (approximately 8,000 and 9,800 light-years). Tycho's SNR has a roughly spherical morphology and spreads over an angular diameter of about 8 arcminutes. Its physical size corresponds to radius of the order of a few parsecs. Its measured expansion rate is about 11â12%/year in radio and X-ray. The average forward shock speed is between 4,000 and 5,000 km/s, dropping to lower speed when encountering local interstellar clouds. Older source list the gas shell has reached an apparent diameter of 3.7 arcminutes.
1935:
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40:
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SN 1572, HR 92, SN 1572A, SNR G120.1+01.4, SNR G120.2+01.4, 1ES 0022+63.8, 1RXS J002509.2+640946, B Cas, BD+63 39a, 8C 0022+638, 4C 63.01, 3C 10, 3C 10.0, 2C 34, RRF 1174, 1XRS 00224+638, 2U 0022+63, 3A 0022+638, 3CR 10, 3U 0022+63, 4U 0022+63, AJG 112, ASB 1, BG 0022+63, CTB 4, KR 101, VRO 63.00.01,
678:
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672:
768:
Tycho G's current velocity is perhaps the strongest evidence that it was the companion star to the white dwarf, as it is traveling at a rate of 136 km/s, which is more than four times faster than the mean velocity of other stars in its stellar neighbourhood. This find has been challenged in
614:
There is no dispute that 3C 10 is the remnant of the supernova observed in 1572â1573. Following a 1964 review article by
Minkowski, the designation 3C 10 appears to be that most commonly used in the literature when referring to the radio remnant of B Cas, although some authors use the tabulated
679:
1691:
Kerzendorf, Wolfgang E.; Yong, David; Schmidt, Brian P.; Simon, Joshua D.; Jeffery, C. Simon; Anderson, Jay; Podsiadlowski, Philipp; Gal-Yam, Avishay; Silverman, Jeffrey M.; Filippenko, Alexei V.; Nomoto, Ken'Ichi; Murphy, Simon J.; Bessell, Michael S.; Venn, Kim A.; Foley, Ryan J. (2013). "A
628:
627:
624:
629:
676:
1573:
Hayato, Asami; Yamaguchi, Hiroya; Tamagawa, Toru; Katsuda, Satoru; Hwang, Una; Hughes, John
Patrick; Ozawa, Midori; Bamba, Aya; Kinugasa, Kenzo (2010). "Expansion Velocity of Ejecta in Tycho's Supernova Remnant Measured by Doppler Broadened X-ray Line Emission".
396:
in 1602 and 1610), a work containing both Brahe's own observations and the analysis of sightings from many other observers. Comparisons between Brahe's observations and those of
Spanish scientist Jerónimo Muñoz revealed that the object was more distant than the
626:
488:
when that planet was at its brightest. Contrarily, Brahe described the supernova as "brighter than Venus". The supernova remained visible to the naked eye into early 1574, gradually fading until it disappeared from view.
625:
675:
619:. Because the radio remnant was reported before the optical supernova-remnant wisps were discovered, the designation 3C 10 is used by some to signify the remnant at all wavelengths.
646:
X-ray observatory at 4U 0022+63. Earlier catalog designations are X120+2 and XRS 00224+638. Cepheus X-1 is actually in the constellation
Cassiopeia, and it is SN 1572, the Tycho
426:
787:
light-years away, on the lower end of SN 1572's possible range of distances, which in turn lowered the calculated velocity from 136 km/s to only 56 km/s.
1496:
Williams, Brian J; Chomiuk, Laura; Hewitt, John W; Blondin, John M; Borkowski, Kazimierz J; Ghavamian, Parviz; Petre, Robert; Reynolds, Stephen P (April 6, 2016).
313:, one of eight supernovae visible to the naked eye in historical records. It appeared in early November 1572 and was independently discovered by many individuals.
1745:
823:, Don Olson and Russell Doescher of the Physics Department and Marilynn Olson of the English Department, argued that this supernova is described in Shakespeare's
2269:
480:
The more reliable contemporary reports state that the new star itself burst forth soon after
November 2, 1572 and by November 11 it was already brighter than
2580:
599:. This was confirmed, and its position more accurately measured in 1957 by Baldwin and Edge using the Cambridge Radio Telescope working at a wavelength of
761:
that ultimately resulted in the supernova. A subsequent study, published in March 2005, revealed further details about this star: Tycho G was probably a
477:: in accordance with the cosmological tradition, the emperor was warned to consider his misbehavior, since the new star was interpreted as an evil omen.
521:, but its detailed classification within the type Ia class continued to be debated until the spectrum of its light at peak luminosity was measured in a
1302:
3684:
731:. A shell of gas is still expanding from its center at about 9,000 km/s. A recent study indicates a rate of expansion below 5,000 km/s.
1198:
Tian, Wenwu; Leahy, Denis A. (December 26, 2010). "Tycho SN 1572: A Naked Ia
Supernova Remnant without Associated Ambient Molecular Cloud".
2484:
1002:"Libro del nuevo Cometa, y del lugar donde se hazen; y como se vera por las Parallaxes quan lexos estan de tierra; y del Prognostico deste"
604:
608:
484:. Around November 16, 1572, it reached its peak brightness at about magnitude −4.0, with some descriptions giving it as equal to
769:
recent years. The star is relatively far away from the center and does not show rotation which might be expected of a companion star.
2573:
765:
or subgiant before the explosion, but some of its mass was stripped away and its outer layers were shock-heated by the supernova.
2464:
898:
Krause, Oliver; et al. (2008). "Tycho Brahe's 1572 supernova as a standard type Ia as revealed by its light-echo spectrum".
3694:
2072:
528:
The classification as a type Ia supernova of normal luminosity allows an accurate measure of the distance to SN 1572. The peak
392:("Concerning the Star, new and never before seen in the life or memory of anyone", published in 1573 with reprints overseen by
1786:
1280:
984:
261:
17:
1861:
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361:
supernova of 1572 belongs among the most important observation events in the history of astronomy. The appearance of the "
3679:
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2566:
2479:
663:
1048:
De mirabili Novae ac splendidis stellae, Mense
Nouembri anni 1572, primum conspectĂŠ, ac etiam nunc apparentis, PhĆnomeno
1753:
369:
and to speed on a revolution in astronomy that began with the realisation of the need to produce better astrometric
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1924:
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1984:
1831:
444:
431:
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2600:
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2504:
2012:
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2305:
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1914:
872:
452:
341:
310:
142:
102:
67:
2840:
1969:
1894:
1103:
63:
52:
3669:
2489:
1854:
1627:
Ruiz-Lapuente, Pilar; et al. (2004). "The binary progenitor of Tycho Brahe's 1572 supernova".
596:
414:
405:
as an astronomical body as well. Other
Europeans to sight the supernova included Wolfgang Schuler,
3054:
3049:
2514:
1919:
1909:
1019:
856:
73:
373:, and thus the need for more precise astronomical observing instruments. It also challenged the
3689:
3011:
2519:
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2259:
2132:
2112:
1749:
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soon after type I and type II supernovae were first defined on the basis of their spectra. The
448:
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320:
has been observed optically but was first detected at radio wavelengths. It is often known as
3350:
2948:
2938:
2762:
2363:
2310:
1964:
1776:
1061:
1433:
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2732:
2727:
2122:
1959:
1711:
1646:
1593:
1519:
1498:"An X-ray and Radio Study of the Varying Expansion Velocities in Tycho's Supernova Remnant"
1468:
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919:
588:
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1934:
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8:
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2702:
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2154:
2144:
2127:
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1991:
1847:
1455:
Wood, KS; Meekins, JF; Yentis, DJ; Smathers, HW; McNutt, DP; Bleach, RD (December 1984).
1098:
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1207:
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1112:
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909:
815:
762:
541:
529:
216:
160:
1605:
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1229:
1160:
501:
Light curve of Tycho's supernova, reconstructed from historical observations (via the
230:[DGW65] 3, PBC J0024.9+6407, F3R 3628, WB 0022+6351, CGPSE 107, GB6 B0022+6352
3409:
2752:
2717:
2677:
2667:
2647:
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2170:
2100:
2037:
1949:
1899:
1884:
1782:
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1723:
1692:
High-resolution
Spectroscopic Search for the Remaining Donor for Tycho's Supernova".
1662:
1613:
1559:
1547:
1417:
1276:
1237:
980:
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720:
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688:
647:
643:
518:
317:
303:
132:
44:
1142:
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2918:
2913:
2908:
2903:
2893:
2888:
2672:
2657:
2637:
2209:
2017:
2007:
1719:
1674:
1654:
1601:
1537:
1527:
1476:
1437:
1363:
1351:
1268:
1225:
1180:
1130:
947:
927:
900:
844:
741:
366:
362:
1821:
2747:
2742:
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2722:
2712:
2662:
2117:
2022:
1811:
1272:
974:
837:
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393:
109:
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2800:
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2707:
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2149:
2105:
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and explodes. This type of supernova does not typically create the spectacular
370:
350:
3070:
2558:
1334:(1952). "Radio-Frequency Radiation from Tycho Brahe's Supernova (A.D. 1572)".
658:
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474:
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307:
97:
1817:
NASA Astronomy
Picture of the Day: Tycho's Supernova Remnant (17 March 2009)
1001:
571:
The distance to the supernova remnant has been estimated to between 2 and 5
82:
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2182:
1816:
1666:
1551:
1331:
1156:
1024:
939:
592:
466:
746:
3494:
3489:
3212:
3181:
3176:
3171:
3166:
3161:
3156:
3151:
3146:
3100:
2433:
2341:
2236:
2226:
2214:
2139:
2052:
1641:
1117:
796:
758:
728:
708:
615:
galactic designation G120.7+2.1 and many authors commonly refer to it as
576:
510:
459:
440:
385:
345:
285:
119:
1658:
931:
642:
An X-ray source designated Cepheus X-1 (or Cep X-1) was detected by the
3327:
3207:
3141:
2448:
2443:
2438:
2418:
2219:
2095:
2057:
1954:
1047:
970:
966:
572:
522:
447:
come and visit "to have his advice about the new star that appeared in
204:
156:
39:
757:. It is thought to be the companion star that contributed mass to the
509:
The supernova was classified as type I on the basis of its historical
384:
The supernova of 1572 is often called "Tycho's supernova", because of
270:
3136:
3128:
3075:
3044:
3039:
3001:
2996:
2991:
2933:
2898:
2428:
2408:
2403:
2398:
2393:
2348:
2042:
1979:
1974:
1904:
1870:
1379:"Radio emission from the remnants of the supernovae of 1572 and 1604"
1355:
833:
456:
358:
299:
181:
525:
in 2008. This gave final confirmation that it was a normal type Ia.
497:
3514:
3509:
3414:
3363:
3322:
3317:
3312:
3034:
3029:
2986:
2981:
2923:
2413:
2378:
2373:
2368:
2192:
2032:
1514:
1481:
1456:
1251:
Decourchelle, Anne (2017), Alsabti, Athem W.; Murdin, Paul (eds.),
1184:
1134:
1020:"Blast From The Past: Astronomers Resurrect 16th-Century Supernova"
773:
336:
1706:
1588:
1212:
914:
711:
star has accreted matter from a companion until it approaches the
3540:
3458:
3453:
3448:
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3358:
3307:
3302:
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3287:
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3272:
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3257:
3252:
3247:
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3217:
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3024:
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2956:
2388:
2336:
1827:
The Search for the Companion Star of Tycho Brahe's 1572 Supernova
1804:
754:
724:
481:
344:
showing the position (labelled I) of the supernova of 1572. From
248:
238:
699:. It was later photographed by a telescope on the international
502:
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3404:
3394:
3341:
2976:
2971:
2966:
2928:
2383:
2187:
825:
716:
696:
587:
The search for a supernova remnant was futile until 1952, when
517:
spectrum of the remnant showed that it was almost certainly of
257:
171:
1572:
1101:(2004). "Tycho Brahe's Supernova: Light from Centuries Past".
595:
reported a radio detection at 158.5 MHz, obtained at the
3504:
3484:
3479:
3379:
3090:
1839:
1259:, Cham: Springer International Publishing, pp. 117â137,
809:
associates the appearance of the supernova with the youthful
700:
514:
485:
48:
1495:
851:" casually mentions the supernova. It is a major element in
3499:
3110:
3105:
2615:
2047:
455:... to which he gave his judgement very learnedly", as the
398:
3597:
1690:
691:
of B Cas was discovered in the 1960s by scientists with a
1746:"Researchers say star in Hamlet may be supernova of 1572"
1454:
750:
683:
Expansion of Tycho's Supernova Remnant from 2000 to 2015
2270:
Timeline of white dwarfs, neutron stars, and supernovae
1420:(September 1964). "Supernovae and Supernova Remnants".
324:, a radio-source designation, although increasingly as
662:
The red circle visible in the upper left part of this
3574:
607:
as object "2C 34", and more firmly as "3C 10" in the
603:. The remnant was also identified tentatively in the
532:
can be calculated from the B-band decline rate to be
1326:
3531:
390:De nova et nullius aevi memoria prius visa stella
3646:
703:spacecraft. The supernova has been confirmed as
2588:
1832:cnn.com: Important days in history of universe
829:, specifically by Bernardo in Act I, Scene i.
2574:
1855:
1805:Light curve and spectrum of Tycho's Supernova
1686:
1684:
1626:
1097:
3198:
2485:Monte Agliale Supernovae and Asteroid Survey
1250:
893:
891:
889:
887:
1422:Annual Review of Astronomy and Astrophysics
1376:
965:
605:second Cambridge Catalogue of Radio Sources
462:recorded in his memoranda a century later.
2581:
2567:
1862:
1848:
1781:. Rowman & Littlefield. pp. 41â.
1681:
1060:Aubrey, John (1898). Clark, Andrew (ed.).
582:
72:
38:
3127:
1705:
1640:
1587:
1541:
1531:
1513:
1480:
1416:
1211:
1197:
1116:
913:
884:
666:infrared image is the remnant of SN 1572.
27:Supernova in the constellation Cassiopeia
1161:"B Cassiopeiae as a Supernova of Type I"
669:
657:
621:
496:
469:China, the star became an issue between
335:
3685:Astronomical objects discovered in 1572
331:
14:
3647:
1774:
1253:"Supernova of 1572, Tycho's Supernova"
1093:
1091:
1059:
979:. New York: Random House. p. 33.
897:
2562:
1900:Type II (IIP, IIL, IIn, and IIb)
1843:
1155:
999:
443:had the mathematician and astrologer
379:unchangeability of the realm of stars
2543:
1778:Edgar Allan Poe: His Life and Legacy
1448:
1377:Baldwin, J. E.; Edge, D. O. (1957).
1149:
961:
959:
957:
813:, and in the November 1998 issue of
653:
637:
566:
2480:Katzman Automatic Imaging Telescope
1457:"The HEAO A-1 X-ray source catalog"
1442:10.1146/annurev.aa.02.090164.001335
1088:
24:
401:. This lead Brahe to approach the
25:
3716:
1798:
1077:Science and Civilization in China
954:
832:The supernova inspired the poem "
734:
633:Tour of Tycho's Supernova remnant
3632:
3620:
3608:
3596:
3584:
3561:
3560:
2542:
2533:
2532:
2265:History of supernova observation
1933:
1066:. Oxford: Clarendon. p. 28.
821:Southwest Texas State University
790:
776:, the star was calculated to be
340:A star map of the constellation
256:
163:) and 9,800 ly (3 kpc)
2606:Cassiopeia in Chinese astronomy
1768:
1738:
1620:
1566:
1489:
1410:
1401:
1370:
1320:
1295:
1244:
1191:
1082:1587, a Year of No Significance
861:Galaxy Science Fiction Magazine
2510:SuperNova Early Warning System
1925:Common envelope jets supernova
1869:
1752:. June 8, 2016. Archived from
1070:
1053:
1040:
1012:
993:
540:. Given estimates of the peak
13:
1:
3695:Bright Star Catalogue objects
1200:Astrophysical Journal Letters
878:
749:, similar in type to our own
739:In October 2004, a letter in
367:ancient models of the heavens
2500:Supernova/Acceleration Probe
2475:High-Z Supernova Search Team
2073:pulsational pair-instability
1822:solstation.com: Tycho's Star
1303:"SN 1572, Tycho's Supernova"
1273:10.1007/978-3-319-21846-5_48
1063:Aubrey's Brief Lives, Vol. 1
745:reported the discovery of a
552:magnitudes, the distance is
544:and the known extinction of
492:
7:
2601:List of stars in Cassiopeia
2590:Constellation of Cassiopeia
2505:Supernova Cosmology Project
2013:Fast blue optical transient
1606:10.1088/0004-637X/725/1/894
1533:10.3847/2041-8205/823/2/L32
1230:10.1088/2041-8205/729/2/L15
866:
855:'s spoof science article, "
10:
3721:
3680:Cassiopeia (constellation)
1724:10.1088/0004-637X/774/2/99
873:List of supernova remnants
695:telescope as a very faint
575:(approx. 6,500 and 16,300
68:astrophysical X-ray source
3558:
3527:
3467:
3441:
3432:
3372:
3349:
3340:
3194:
3123:
3063:
3010:
2947:
2839:
2761:
2623:
2614:
2596:
2528:
2457:
2319:
2278:
2252:
2163:
2088:
2000:
1942:
1931:
1877:
1694:The Astrophysical Journal
1576:The Astrophysical Journal
1502:The Astrophysical Journal
1104:The Astrophysical Journal
819:, three researchers from
617:Tycho's supernova remnant
326:Tycho's supernova remnant
267:
254:
244:
234:
225:
214:
203:
195:
187:
177:
167:
151:
141:
131:
118:
108:
96:
88:
81:
64:Astronomical radio source
59:
53:Chandra X-ray Observatory
37:
2490:Nearby Supernova Factory
1775:Meyers, Jeffrey (2000).
1461:Astrophys. J. Suppl. Ser
1000:Muñoz, Jerónimo (1573).
795:In the ninth episode of
597:Jodrell Bank Observatory
262:Related media on Commons
2515:Supernova Legacy Survey
1434:1964ARA&A...2..247M
857:The Martian Star-Gazers
583:Initial radio detection
3700:Durchmusterung objects
2520:Texas Supernova Search
2495:Sloan Supernova Survey
2113:Luminous blue variable
1750:Texas State University
1257:Handbook of Supernovae
859:", first published in
684:
667:
634:
506:
503:Open Supernova Catalog
427:BartholomÀus Reisacher
357:The appearance of the
354:
47:of SN 1572 as seen in
18:Tycho's supernova
3655:Historical supernovae
1965:Phillips relationship
1165:Astrophysical Journal
847:'s 1955 short story "
682:
661:
632:
500:
339:
1756:on September 6, 2008
1099:Ruiz-Lapuente, Pilar
1079:, v.3 pp.425-6; cf.
609:third Cambridge list
589:Robert Hanbury Brown
332:Historic description
143:Galactic coordinates
3533:Astronomical events
2538:Category:Supernovae
2470:CalĂĄn/Tololo Survey
2155:Population III star
2063:Soft gamma repeater
1895:Type Ib and Ic
1716:2013ApJ...774...99K
1659:10.1038/nature03006
1651:2004Natur.431.1069R
1635:(7012): 1069â1072.
1598:2010ApJ...725..894H
1524:2016ApJ...823L..32W
1473:1984ApJS...56..507W
1395:1957Obs....77..139B
1348:1952Natur.170..364H
1265:2017hsn..book..117D
1222:2011ApJ...729L..15T
1177:1945ApJ...102..309B
1127:2004ApJ...612..357R
932:10.1038/nature07608
924:2008Natur.456..617K
843:The protagonist in
816:Sky & Telescope
811:William Shakespeare
713:Chandrasekhar limit
419:Francesco Maurolico
407:Christopher Clavius
403:Great Comet of 1577
365:" helped to revise
155:between 8,000
34:
3660:Supernova remnants
2548:Commons:Supernovae
2200:Stellar black hole
2176:Pulsar wind nebula
2028:Gravitational wave
1810:2018-10-31 at the
1407:(Edge et al. 1959)
1028:. December 4, 2008
763:main-sequence star
727:which created the
721:Type II supernovas
685:
668:
635:
542:apparent magnitude
530:absolute magnitude
507:
388:'s extensive work
355:
226:Other designations
217:apparent magnitude
32:
3572:
3571:
3554:
3553:
3523:
3522:
3428:
3427:
3336:
3335:
3190:
3189:
3119:
3118:
2556:
2555:
2171:Supernova remnant
2038:Luminous red nova
1950:Carbon detonation
1788:978-0-8154-1038-6
1342:(4322): 364â365.
1328:Hanbury Brown, R.
1282:978-3-319-21846-5
986:978-0-3078-0105-0
908:(7222): 617â619.
689:supernova remnant
680:
654:Optical detection
638:X-ray observation
630:
567:Supernova remnant
318:supernova remnant
278:
277:
16:(Redirected from
3712:
3637:
3636:
3635:
3625:
3624:
3623:
3613:
3612:
3611:
3601:
3600:
3589:
3588:
3587:
3580:
3564:
3563:
3529:
3528:
3439:
3438:
3410:LBN 114.55+00.22
3347:
3346:
3196:
3195:
3125:
3124:
3035:17156 (Nushagak)
2621:
2620:
2583:
2576:
2569:
2560:
2559:
2546:
2545:
2536:
2535:
2399:Remnant G1.9+0.3
2018:Fast radio burst
1937:
1915:Pair-instability
1864:
1857:
1850:
1841:
1840:
1793:
1792:
1772:
1766:
1765:
1763:
1761:
1742:
1736:
1735:
1709:
1688:
1679:
1678:
1644:
1642:astro-ph/0410673
1624:
1618:
1617:
1591:
1570:
1564:
1563:
1545:
1535:
1517:
1493:
1487:
1486:
1484:
1452:
1446:
1445:
1414:
1408:
1405:
1399:
1398:
1374:
1368:
1367:
1356:10.1038/170364a0
1324:
1318:
1317:
1315:
1313:
1299:
1293:
1292:
1291:
1289:
1248:
1242:
1241:
1215:
1195:
1189:
1188:
1153:
1147:
1146:
1120:
1118:astro-ph/0309009
1095:
1086:
1074:
1068:
1067:
1057:
1051:
1044:
1038:
1037:
1035:
1033:
1016:
1010:
1009:
997:
991:
990:
963:
952:
951:
917:
895:
845:Arthur C. Clarke
786:
785:
784:
719:more typical of
693:Palomar Mountain
681:
631:
602:
562:
561:
560:
551:
549:
539:
537:
435:
271:edit on Wikidata
260:
127:
77:
76:
42:
35:
31:
21:
3720:
3719:
3715:
3714:
3713:
3711:
3710:
3709:
3670:1572 in science
3645:
3644:
3643:
3633:
3631:
3621:
3619:
3609:
3607:
3595:
3585:
3583:
3575:
3573:
3568:
3550:
3519:
3463:
3424:
3368:
3332:
3186:
3115:
3081:IRAS 23304+6147
3059:
3006:
2943:
2835:
2757:
2610:
2592:
2587:
2557:
2552:
2524:
2453:
2439:SN 2016aps
2419:SN Refsdal
2315:
2274:
2248:
2159:
2145:WolfâRayet star
2084:
2023:Gamma-ray burst
1996:
1970:Nucleosynthesis
1938:
1929:
1873:
1868:
1837:
1812:Wayback Machine
1801:
1796:
1789:
1773:
1769:
1759:
1757:
1744:
1743:
1739:
1689:
1682:
1625:
1621:
1571:
1567:
1494:
1490:
1467:(12): 507â649.
1453:
1449:
1415:
1411:
1406:
1402:
1383:The Observatory
1375:
1371:
1325:
1321:
1311:
1309:
1307:spider.seds.org
1301:
1300:
1296:
1287:
1285:
1283:
1249:
1245:
1196:
1192:
1154:
1150:
1096:
1089:
1075:
1071:
1058:
1054:
1045:
1041:
1031:
1029:
1018:
1017:
1013:
998:
994:
987:
964:
955:
896:
885:
881:
869:
838:Edgar Allan Poe
807:Stephen Dedalus
793:
782:
780:
779:
777:
737:
670:
656:
640:
622:
600:
585:
569:
558:
556:
555:
553:
547:
545:
535:
533:
495:
441:Queen Elizabeth
429:
394:Johannes Kepler
371:star catalogues
334:
298:(B Cas), was a
274:
196:Progenitor type
125:
110:Right ascension
71:
55:
51:light from the
28:
23:
22:
15:
12:
11:
5:
3718:
3708:
3707:
3702:
3697:
3692:
3687:
3682:
3677:
3672:
3667:
3662:
3657:
3642:
3641:
3629:
3617:
3605:
3593:
3570:
3569:
3559:
3556:
3555:
3552:
3551:
3549:
3548:
3543:
3537:
3535:
3525:
3524:
3521:
3520:
3518:
3517:
3512:
3507:
3502:
3497:
3492:
3487:
3482:
3477:
3471:
3469:
3465:
3464:
3462:
3461:
3456:
3451:
3445:
3443:
3436:
3430:
3429:
3426:
3425:
3423:
3422:
3417:
3412:
3407:
3402:
3397:
3392:
3387:
3382:
3376:
3374:
3370:
3369:
3367:
3366:
3361:
3355:
3353:
3344:
3338:
3337:
3334:
3333:
3331:
3330:
3325:
3320:
3315:
3310:
3305:
3300:
3295:
3290:
3285:
3280:
3275:
3270:
3265:
3260:
3255:
3250:
3245:
3240:
3235:
3230:
3225:
3220:
3215:
3210:
3204:
3202:
3192:
3191:
3188:
3187:
3185:
3184:
3179:
3174:
3169:
3164:
3159:
3154:
3149:
3144:
3139:
3133:
3131:
3121:
3120:
3117:
3116:
3114:
3113:
3108:
3103:
3098:
3093:
3091:PSR J0205+6449
3088:
3083:
3078:
3073:
3067:
3065:
3061:
3060:
3058:
3057:
3052:
3047:
3042:
3037:
3032:
3027:
3022:
3016:
3014:
3008:
3007:
3005:
3004:
2999:
2994:
2989:
2984:
2979:
2974:
2969:
2964:
2959:
2953:
2951:
2945:
2944:
2942:
2941:
2936:
2931:
2926:
2921:
2916:
2911:
2906:
2901:
2896:
2891:
2886:
2881:
2876:
2871:
2866:
2861:
2856:
2851:
2845:
2843:
2837:
2836:
2834:
2833:
2828:
2823:
2818:
2813:
2808:
2803:
2798:
2793:
2788:
2783:
2778:
2773:
2767:
2765:
2759:
2758:
2756:
2755:
2750:
2745:
2740:
2735:
2730:
2725:
2720:
2715:
2710:
2705:
2700:
2695:
2690:
2685:
2680:
2675:
2670:
2665:
2660:
2655:
2650:
2645:
2640:
2635:
2629:
2627:
2618:
2612:
2611:
2609:
2608:
2603:
2597:
2594:
2593:
2586:
2585:
2578:
2571:
2563:
2554:
2553:
2551:
2550:
2540:
2529:
2526:
2525:
2523:
2522:
2517:
2512:
2507:
2502:
2497:
2492:
2487:
2482:
2477:
2472:
2467:
2461:
2459:
2455:
2454:
2452:
2451:
2446:
2441:
2436:
2431:
2429:SN 2006gy
2426:
2421:
2416:
2411:
2409:SN 2011fe
2406:
2404:SN 2007bi
2401:
2396:
2394:SN 2003fg
2391:
2386:
2381:
2376:
2371:
2366:
2361:
2356:
2351:
2346:
2345:
2344:
2334:
2329:
2327:Barnard's Loop
2323:
2321:
2317:
2316:
2314:
2313:
2308:
2303:
2298:
2293:
2288:
2282:
2280:
2276:
2275:
2273:
2272:
2267:
2262:
2256:
2254:
2250:
2249:
2247:
2246:
2245:
2244:
2242:OrionâEridanus
2234:
2229:
2224:
2223:
2222:
2217:
2212:
2202:
2197:
2196:
2195:
2190:
2180:
2179:
2178:
2167:
2165:
2161:
2160:
2158:
2157:
2152:
2150:Super-AGB star
2147:
2142:
2137:
2136:
2135:
2130:
2125:
2115:
2110:
2109:
2108:
2103:
2092:
2090:
2086:
2085:
2083:
2082:
2080:Symbiotic nova
2077:
2076:
2075:
2065:
2060:
2055:
2050:
2045:
2040:
2035:
2030:
2025:
2020:
2015:
2010:
2004:
2002:
1998:
1997:
1995:
1994:
1989:
1988:
1987:
1982:
1977:
1967:
1962:
1957:
1952:
1946:
1944:
1940:
1939:
1932:
1930:
1928:
1927:
1922:
1917:
1912:
1907:
1902:
1897:
1892:
1887:
1881:
1879:
1875:
1874:
1867:
1866:
1859:
1852:
1844:
1835:
1834:
1829:
1824:
1819:
1814:
1800:
1799:External links
1797:
1795:
1794:
1787:
1767:
1737:
1680:
1619:
1582:(1): 894â903.
1565:
1488:
1482:10.1086/190992
1447:
1428:(1): 247â266.
1409:
1400:
1369:
1319:
1294:
1281:
1243:
1190:
1185:10.1086/144761
1148:
1135:10.1086/422419
1111:(1): 357â363.
1087:
1069:
1052:
1039:
1011:
992:
985:
953:
882:
880:
877:
876:
875:
868:
865:
792:
789:
736:
735:Companion star
733:
655:
652:
639:
636:
584:
581:
568:
565:
494:
491:
473:and the young
351:De nova stella
333:
330:
276:
275:
268:
265:
264:
252:
251:
246:
242:
241:
236:
232:
231:
227:
223:
222:
219:
212:
211:
208:
201:
200:
197:
193:
192:
189:
185:
184:
179:
175:
174:
169:
165:
164:
153:
149:
148:
145:
139:
138:
135:
129:
128:
122:
116:
115:
112:
106:
105:
100:
94:
93:
90:
86:
85:
79:
78:
61:
57:
56:
43:
26:
9:
6:
4:
3:
2:
3717:
3706:
3703:
3701:
3698:
3696:
3693:
3691:
3690:Bayer objects
3688:
3686:
3683:
3681:
3678:
3676:
3673:
3671:
3668:
3666:
3663:
3661:
3658:
3656:
3653:
3652:
3650:
3640:
3630:
3628:
3618:
3616:
3606:
3604:
3599:
3594:
3592:
3582:
3581:
3578:
3567:
3557:
3547:
3544:
3542:
3539:
3538:
3536:
3534:
3530:
3526:
3516:
3513:
3511:
3508:
3506:
3503:
3501:
3498:
3496:
3493:
3491:
3488:
3486:
3483:
3481:
3478:
3476:
3475:Andromeda VII
3473:
3472:
3470:
3466:
3460:
3457:
3455:
3452:
3450:
3447:
3446:
3444:
3440:
3437:
3435:
3431:
3421:
3418:
3416:
3413:
3411:
3408:
3406:
3403:
3401:
3398:
3396:
3393:
3391:
3388:
3386:
3383:
3381:
3378:
3377:
3375:
3371:
3365:
3362:
3360:
3357:
3356:
3354:
3352:
3348:
3345:
3343:
3339:
3329:
3326:
3324:
3321:
3319:
3316:
3314:
3311:
3309:
3306:
3304:
3301:
3299:
3296:
3294:
3291:
3289:
3286:
3284:
3281:
3279:
3276:
3274:
3271:
3269:
3266:
3264:
3261:
3259:
3256:
3254:
3251:
3249:
3246:
3244:
3241:
3239:
3236:
3234:
3231:
3229:
3226:
3224:
3221:
3219:
3216:
3214:
3211:
3209:
3206:
3205:
3203:
3201:
3200:Star clusters
3197:
3193:
3183:
3180:
3178:
3175:
3173:
3170:
3168:
3165:
3163:
3160:
3158:
3155:
3153:
3150:
3148:
3145:
3143:
3140:
3138:
3135:
3134:
3132:
3130:
3126:
3122:
3112:
3109:
3107:
3104:
3102:
3099:
3097:
3094:
3092:
3089:
3087:
3084:
3082:
3079:
3077:
3074:
3072:
3069:
3068:
3066:
3062:
3056:
3053:
3051:
3048:
3046:
3043:
3041:
3038:
3036:
3033:
3031:
3028:
3026:
3023:
3021:
3018:
3017:
3015:
3013:
3009:
3003:
3000:
2998:
2995:
2993:
2990:
2988:
2985:
2983:
2980:
2978:
2975:
2973:
2970:
2968:
2965:
2963:
2960:
2958:
2955:
2954:
2952:
2950:
2946:
2940:
2937:
2935:
2932:
2930:
2927:
2925:
2922:
2920:
2917:
2915:
2912:
2910:
2907:
2905:
2902:
2900:
2897:
2895:
2892:
2890:
2887:
2885:
2882:
2880:
2877:
2875:
2872:
2870:
2867:
2865:
2862:
2860:
2857:
2855:
2852:
2850:
2847:
2846:
2844:
2842:
2838:
2832:
2829:
2827:
2824:
2822:
2819:
2817:
2814:
2812:
2809:
2807:
2804:
2802:
2799:
2797:
2794:
2792:
2789:
2787:
2784:
2782:
2779:
2777:
2774:
2772:
2769:
2768:
2766:
2764:
2760:
2754:
2751:
2749:
2746:
2744:
2741:
2739:
2736:
2734:
2731:
2729:
2726:
2724:
2721:
2719:
2716:
2714:
2711:
2709:
2706:
2704:
2701:
2699:
2696:
2694:
2691:
2689:
2686:
2684:
2681:
2679:
2676:
2674:
2671:
2669:
2666:
2664:
2661:
2659:
2656:
2654:
2651:
2649:
2646:
2644:
2643:Îł (Navi/Tsih)
2641:
2639:
2636:
2634:
2631:
2630:
2628:
2626:
2622:
2619:
2617:
2613:
2607:
2604:
2602:
2599:
2598:
2595:
2591:
2584:
2579:
2577:
2572:
2570:
2565:
2564:
2561:
2549:
2541:
2539:
2531:
2530:
2527:
2521:
2518:
2516:
2513:
2511:
2508:
2506:
2503:
2501:
2498:
2496:
2493:
2491:
2488:
2486:
2483:
2481:
2478:
2476:
2473:
2471:
2468:
2466:
2463:
2462:
2460:
2456:
2450:
2447:
2445:
2442:
2440:
2437:
2435:
2432:
2430:
2427:
2425:
2422:
2420:
2417:
2415:
2414:SN 2014J
2412:
2410:
2407:
2405:
2402:
2400:
2397:
2395:
2392:
2390:
2387:
2385:
2382:
2380:
2379:SN 1994D
2377:
2375:
2374:SN 1987A
2372:
2370:
2369:SN 1885A
2367:
2365:
2362:
2360:
2357:
2355:
2352:
2350:
2347:
2343:
2340:
2339:
2338:
2335:
2333:
2330:
2328:
2325:
2324:
2322:
2318:
2312:
2309:
2307:
2304:
2302:
2299:
2297:
2296:Massive stars
2294:
2292:
2289:
2287:
2284:
2283:
2281:
2277:
2271:
2268:
2266:
2263:
2261:
2258:
2257:
2255:
2251:
2243:
2240:
2239:
2238:
2235:
2233:
2230:
2228:
2225:
2221:
2218:
2216:
2213:
2211:
2208:
2207:
2206:
2203:
2201:
2198:
2194:
2191:
2189:
2186:
2185:
2184:
2181:
2177:
2174:
2173:
2172:
2169:
2168:
2166:
2162:
2156:
2153:
2151:
2148:
2146:
2143:
2141:
2138:
2134:
2131:
2129:
2126:
2124:
2121:
2120:
2119:
2116:
2114:
2111:
2107:
2104:
2102:
2099:
2098:
2097:
2094:
2093:
2091:
2087:
2081:
2078:
2074:
2071:
2070:
2069:
2066:
2064:
2061:
2059:
2056:
2054:
2051:
2049:
2046:
2044:
2041:
2039:
2036:
2034:
2031:
2029:
2026:
2024:
2021:
2019:
2016:
2014:
2011:
2009:
2006:
2005:
2003:
1999:
1993:
1990:
1986:
1983:
1981:
1978:
1976:
1973:
1972:
1971:
1968:
1966:
1963:
1961:
1958:
1956:
1953:
1951:
1948:
1947:
1945:
1941:
1936:
1926:
1923:
1921:
1918:
1916:
1913:
1911:
1910:Superluminous
1908:
1906:
1903:
1901:
1898:
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1890:Type Iax
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1427:
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1419:
1418:Minkowski, R.
1413:
1404:
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1157:Baade, Walter
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864:
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854:
853:Frederik Pohl
850:
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841:
839:
835:
830:
828:
827:
822:
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808:
804:
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791:In literature
788:
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766:
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732:
730:
726:
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718:
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707:, in which a
706:
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531:
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475:Wanli Emperor
472:
471:Zhang Juzheng
468:
463:
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454:
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442:
437:
433:
428:
424:
420:
416:
412:
411:Thomas Digges
408:
404:
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395:
391:
387:
382:
380:
377:dogma of the
376:
372:
368:
364:
360:
353:
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347:
343:
338:
329:
327:
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319:
314:
312:
309:
308:constellation
305:
301:
297:
296:B Cassiopeiae
293:
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136:
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99:
98:Constellation
95:
92:November 1572
91:
87:
84:
80:
75:
69:
65:
62:
58:
54:
50:
46:
41:
36:
30:
19:
3639:Solar System
3545:
3420:Westerhout 5
3390:Heart Nebula
3385:Cassiopeia A
3086:LS I +61 303
2424:Vela Remnant
2389:SN 1006
2358:
2354:SN 1000+0216
2332:Cassiopeia A
2301:Most distant
2232:Local Bubble
2205:Compact star
2183:Neutron star
1920:Calcium-rich
1885:Type Ia
1836:
1777:
1770:
1758:. Retrieved
1754:the original
1740:
1697:
1693:
1632:
1628:
1622:
1579:
1575:
1568:
1505:
1501:
1491:
1464:
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1412:
1403:
1386:
1382:
1372:
1339:
1335:
1322:
1310:. Retrieved
1306:
1297:
1286:, retrieved
1256:
1246:
1203:
1199:
1193:
1168:
1164:
1151:
1108:
1102:
1080:
1076:
1072:
1062:
1055:
1046:
1042:
1030:. Retrieved
1025:ScienceDaily
1023:
1014:
1005:
995:
975:
905:
899:
860:
842:
831:
824:
814:
800:
794:
771:
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740:
738:
686:
641:
616:
613:
593:Cyril Hazard
586:
570:
527:
508:
479:
467:Ming dynasty
464:
445:Thomas Allen
439:In England,
438:
423:TadeĂĄĆĄ HĂĄjek
389:
383:
375:Aristotelian
356:
349:
325:
321:
315:
295:
292:Tycho's Nova
291:
288:'s Supernova
284:
280:
279:
29:
3675:Tycho Brahe
3627:Outer space
3615:Spaceflight
3546:SN 1572 (B)
3495:Dwingeloo 2
3490:Dwingeloo 1
3213:Messier 103
3182:HD 240237 b
3177:HD 240210 b
3147:HD 219134 b
2733:Ï
(Castula)
2648:ÎŽ (Ruchbah)
2633:α (Schedar)
2434:ASASSN-15lh
2384:SN 185
2342:Crab Nebula
2237:Superbubble
2227:Zombie star
2210:electroweak
2140:White dwarf
2089:Progenitors
2053:Pulsar kick
1760:February 6,
1389:: 139â143.
1008:. Valencia.
1006:Bg/36967(1)
971:Druyan, Ann
967:Sagan, Carl
797:James Joyce
759:white dwarf
729:Crab Nebula
709:white dwarf
577:light-years
511:light curve
460:John Aubrey
430: [
386:Tycho Brahe
346:Tycho Brahe
245:Followed by
235:Preceded by
147:G.120.1+1.4
120:Declination
3705:3C objects
3649:Categories
3328:Trumpler 3
3208:Messier 52
3142:HD 17156 b
3129:Exoplanets
3101:4U 0142+61
3071:BD+60°2522
2668:Ξ (Marfak)
2663:η (Achird)
2449:SN 2022jli
2444:SN 2018cow
2311:In fiction
2286:Candidates
2260:Guest star
2118:Supergiant
2096:Hypergiant
2058:Quark-nova
1960:Near-Earth
1943:Physics of
1871:Supernovae
1515:1604.01779
1508:(2): L32.
1332:Hazard, C.
1206:(2): L15.
1032:January 6,
879:References
753:and named
723:, such as
601:1.9 m
523:light echo
453:Cassiopeia
342:Cassiopeia
311:Cassiopeia
188:Progenitor
159:(2.5
103:Cassiopeia
60:Event type
3591:Astronomy
3137:HD 7924 b
3076:Gliese 49
2763:Flamsteed
2653:Δ (Segin)
2349:iPTF14hls
2253:Discovery
2043:Micronova
1992:Neutrinos
1985:Îł-process
1980:r-process
1975:p-process
1955:Foe/Bethe
1905:Hypernova
1732:118470111
1707:1210.2713
1700:(2): 99.
1614:119102740
1589:1009.6031
1560:118542192
1312:March 10,
1288:March 10,
1238:119104584
1213:1012.5673
915:0810.5106
863:in 1962.
834:Al Aaraaf
493:Supernova
457:antiquary
359:Milky Way
300:supernova
182:Milky Way
3566:Category
3515:Maffei 2
3510:Maffei 1
3434:Galaxies
3415:Sh 2-185
3323:NGC 7790
3318:NGC 7789
3313:NGC 1027
2841:Variable
2658:ζ (Fulu)
2638:ÎČ (Caph)
2458:Research
2364:Kepler's
2306:Remnants
2193:magnetar
2164:Remnants
2068:Imposter
2033:Kilonova
1808:Archived
1667:15510140
1552:32714502
1159:(1945).
1143:15830343
973:(1997).
940:19052622
867:See also
849:The Star
774:Gaia DR2
449:the Swan
415:John Dee
363:new star
152:Distance
3577:Portals
3541:SN 1181
3400:IC 1805
3342:Nebulae
3308:NGC 663
3303:NGC 659
3298:NGC 654
3293:NGC 637
3288:NGC 559
3283:NGC 457
3278:NGC 436
3273:NGC 433
3268:NGC 381
3263:NGC 366
3258:NGC 358
3253:NGC 225
3248:NGC 189
3243:NGC 146
3238:NGC 136
3233:NGC 133
3228:NGC 129
3223:NGC 110
3218:NGC 103
3096:Tycho G
2869:YZ (21)
2465:ASAS-SN
2359:Tycho's
2337:SN 1054
2320:Notable
2291:Notable
2001:Related
1878:Classes
1712:Bibcode
1675:4346227
1647:Bibcode
1594:Bibcode
1543:7380093
1520:Bibcode
1469:Bibcode
1430:Bibcode
1391:Bibcode
1364:4161519
1344:Bibcode
1261:Bibcode
1218:Bibcode
1173:Bibcode
1171:: 309.
1123:Bibcode
948:4409995
920:Bibcode
802:Ulysses
755:Tycho G
747:G2 star
725:SN 1054
705:Type Ia
519:type Ia
482:Jupiter
306:in the
304:Type Ia
281:SN 1572
249:SN 1604
239:SN 1181
199:Unknown
191:Unknown
168:Remnant
124:+64° 09
83:Type Ia
45:Remnant
33:SN 1572
3405:KjPn 8
3395:IC 289
3055:240430
3050:240429
3045:240237
3040:240210
2816:48 (A)
2215:exotic
2188:pulsar
2133:yellow
2101:yellow
2008:Failed
1785:
1730:
1673:
1665:
1629:Nature
1612:
1558:
1550:
1540:
1362:
1336:Nature
1279:
1236:
1141:
983:
969:&
946:
938:
901:Nature
826:Hamlet
783:â1,200
781:+2,000
742:Nature
717:nebula
697:nebula
294:), or
255:
205:Colour
172:Nebula
114:0 25.3
70:
3603:Stars
3505:IC 10
3485:3C 35
3480:3C 20
3468:Other
3380:3C 58
3373:Other
3162:e (h)
3064:Other
3030:15558
2939:V1405
2934:V1022
2625:Bayer
2616:Stars
2279:Lists
2220:quark
1728:S2CID
1702:arXiv
1671:S2CID
1637:arXiv
1610:S2CID
1584:arXiv
1556:S2CID
1510:arXiv
1360:S2CID
1234:S2CID
1208:arXiv
1139:S2CID
1113:arXiv
976:Comet
944:S2CID
910:arXiv
836:" by
778:6,400
701:ROSAT
644:Uhuru
563:kpc.
534:â19.0
515:X-ray
486:Venus
434:]
322:3C 10
286:Tycho
269:[
215:Peak
207:(B-V)
133:Epoch
49:X-ray
3665:1572
3500:MB 3
3364:7635
3111:WR 3
3106:WR 2
3025:7977
3020:7924
3002:8881
2997:8853
2992:8832
2929:V987
2924:V773
2919:V863
2914:V762
2909:V705
2904:V669
2899:V547
2894:V509
2889:V373
2123:blue
2048:Nova
1783:ISBN
1762:2018
1663:PMID
1548:PMID
1314:2023
1290:2023
1277:ISBN
1034:2024
981:ISBN
936:PMID
687:The
664:WISE
591:and
559:â0.9
557:+1.5
546:1.86
425:and
399:Moon
316:Its
178:Host
89:Date
3459:278
3454:185
3449:147
3442:NGC
3359:281
3351:NGC
2987:932
2982:743
2977:297
2972:273
2967:244
2962:196
2957:144
2128:red
2106:Red
1720:doi
1698:774
1655:doi
1633:431
1602:doi
1580:725
1538:PMC
1528:doi
1506:823
1477:doi
1438:doi
1352:doi
1340:170
1269:doi
1226:doi
1204:729
1181:doi
1169:102
1131:doi
1109:612
928:doi
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799:'s
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751:Sun
648:SNR
611:.
573:kpc
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550:0.2
538:0.3
465:In
451:or
348:'s
302:of
161:kpc
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3012:HD
2949:HR
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2859:TZ
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Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
