32:
3006:
39:
1386:
Takeda, Yoichi; et al. (February 2005), "High-Dispersion
Spectra Collection of Nearby F--K Stars at Okayama Astrophysical Observatory: A Basis for Spectroscopic Abundance Standards",
1722:
1158:
Takeda, Genya; et al. (February 2007), "Structure and
Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog",
1747:
Lubin, Dan; Tytler, David; Kirkman, David (March 2012), "Frequency of
Maunder Minimum Events in Solar-type Stars Inferred from Activity and Metallicity Observations",
1714:
2000:
529:
1331:
1661:
Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of
Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)",
2027:
1486:
1102:
Holmberg, J.; et al. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics",
402:
1423:
Mamajek, Eric E.; Hillenbrand, Lynne A. (November 2008), "Improved Age
Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics",
3073:
697:
Lambda
Aurigae has been examined for the presence of excess infrared emission that may indicate the presence of a circumstellar
3083:
1896:
1834:
1010:
Boyajian, Tabetha S.; et al. (February 2012), "Stellar
Diameters and Temperatures. I. Main-sequence A, F, and G Stars",
2020:
3028:
1975:
1267:
Kovtyukh, V. V.; et al. (2003), "High precision effective temperatures for 181 F-K dwarfs from line-depth ratios",
674:, while the mass and radius are slightly larger. It is 73% more luminous than the Sun and radiates this energy from its
1726:
1945:
1857:
513:
1784:
Kovacs, N.; Foy, R. (August 1978), "A detailed analysis of three stars in the Eggen's
Epsilon INDI moving group",
3058:
3009:
2013:
60:
628:
of +66.5 km/s, having come to within 24.4 ly (7.5 pc) some 117,300 years ago. It has a high
3068:
1608:
Bailer-Jones, C.A.L.; et al. (2018), "New stellar encounters discovered in the second Gaia data release",
1506:
574:
1067:
Keenan, Philip C.; McNeil, Raymond C. (1989), "The
Perkins catalog of revised MK types for the cooler stars",
950:
447:
537:
533:
2047:
909:
798:
541:
509:
3078:
3063:
1547:
1269:
710:
1329:
Greaves, J. S.; Wyatt, M. C.; Bryden, G. (August 2009), "Debris discs around nearby solar analogues",
3038:
3033:
2427:
1866:
896:
702:
652:
609:
525:
3043:
659:
of G1 V. It is sometimes listed with a class of G1.5 IV-V Fe-1, which indicates the
2052:
3053:
2648:
2036:
1814:
656:
605:
517:
122:
73:
2808:
2560:
2247:
1826:
1819:
679:
670:
along with a noticeable underabundance of iron. In terms of composition it is similar to the
586:
503:
498:
410:
1797:
1631:
1570:
1476:
1292:
1234:
1211:
Chen, Y. Q.; et al. (February 2000), "Chemical composition of 90 F and G disk dwarfs",
1125:
933:
562:
1793:
1756:
1680:
1627:
1566:
1442:
1395:
1350:
1288:
1230:
1177:
1121:
1076:
1029:
983:
928:
706:
255:
8:
521:
1760:
1684:
1446:
1399:
1354:
1181:
1080:
1033:
987:
2989:
1696:
1670:
1643:
1617:
1582:
1556:
1458:
1432:
1368:
1340:
1304:
1278:
1246:
1220:
1193:
1167:
1137:
1111:
1045:
1019:
918:
843:
811:
675:
276:
105:
1769:
1041:
862:
would have an apparent magnitude of approximately -5.48, about 40 times brighter than
2071:
1892:
1830:
1521:
1500:
1363:
1141:
781:
664:
590:
494:
468:
56:
1647:
1586:
1462:
1372:
1308:
1250:
1197:
1049:
2932:
2722:
1764:
1700:
1688:
1635:
1574:
1450:
1403:
1358:
1296:
1238:
1185:
1129:
1084:
1037:
938:
660:
633:
439:
377:
239:
1912:
AEEA (Activities of
Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 13 日
1911:
1639:
1133:
943:
900:
3048:
2177:
2152:
2099:
1578:
1545:
van Leeuwen, Floor (November 2007), "Validation of the new Hipparcos reduction",
1300:
691:
625:
390:
180:
81:
1923:
2981:
2717:
1595:
974:
Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars",
751:
Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars
701:, but no significant surplus has been observed. It is a possible member of the
486:
247:
227:
215:
1967:
3022:
2237:
2167:
2124:
2114:
2094:
1859:
Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars
770:
738:
667:
639:
629:
601:
204:
68:
2797:
2550:
2545:
2540:
2535:
2525:
2232:
2227:
2222:
2217:
2212:
2207:
2202:
2197:
2192:
2119:
2104:
2084:
1408:
594:
350:
306:
31:
2005:
1242:
38:
2187:
2182:
2172:
2162:
2109:
1675:
1283:
1225:
1172:
859:
803:
698:
687:
432:
158:
147:
136:
94:
624:) distant from the Earth. The star is drifting further away with a high
2963:
2867:
2862:
2857:
2773:
2768:
2763:
2758:
2697:
2520:
2515:
2510:
2500:
2495:
2490:
2485:
2480:
2475:
2470:
2465:
2460:
2455:
2450:
2445:
2410:
2405:
2400:
2395:
2390:
2385:
2380:
2375:
2370:
2365:
2360:
2355:
2350:
2345:
2340:
2335:
2330:
2325:
2320:
2315:
2310:
2305:
2300:
2295:
2290:
2285:
2280:
2275:
2157:
2147:
2142:
2137:
2089:
858:) away. Hypothetically viewed from Lambda Aurigae, Capella's quadruple
851:
762:
734:
617:
363:
323:
262:
168:
2872:
2745:
2440:
2435:
2270:
2265:
2260:
2255:
1561:
2906:
2901:
2841:
2836:
2831:
2826:
2821:
2816:
2783:
2778:
2753:
2681:
2676:
2671:
2666:
2661:
2656:
2638:
2628:
2623:
2618:
2608:
2603:
2598:
2593:
2588:
2583:
2578:
2573:
2568:
2505:
2416:
1692:
1622:
1454:
1189:
1088:
923:
807:
613:
475:
1825:(Reprint ed.). New York, NY: Dover Publications Inc. p.
1437:
1345:
1116:
1024:
2927:
2727:
2712:
2702:
2633:
2613:
2079:
1607:
847:
846:
of 4.71. The closest large neighboring star to Lambda Aurigae is
973:
2958:
2950:
2922:
2886:
2707:
1481:
954:
863:
855:
621:
556:
424:
336:
267:
1009:
905:
Data Release 2: Summary of the contents and survey properties"
2530:
839:
1723:
Commonwealth Scientific and Industrial Research Organisation
1266:
690:. It has a low level of surface activity and is a candidate
2062:
597:
231:
219:
1101:
671:
749:), the Tent. According to the catalogue of stars in the
686:. At this heat, the star glows with the yellow hue of a
1385:
1157:
1062:
1060:
976:
Communications of the Lunar and Planetary Laboratory
1210:
1818:
1746:
1422:
1328:
899:; et al. (Gaia collaboration) (August 2018).
1891:, written by 陳久金. Published by 台灣書房出版有限公司, 2005,
1601:
1388:Publications of the Astronomical Society of Japan
1332:Monthly Notices of the Royal Astronomical Society
1057:
802:, refers to an asterism consisting of λ Aurigae,
3020:
1324:
1322:
1320:
1318:
1153:
1151:
757:were the title for three stars : λ Aur as
2980:
1262:
1260:
1005:
1003:
1001:
999:
997:
866:can be seen at maximum brightness from Earth.
2021:
1487:Centre de données astronomiques de Strasbourg
1416:
1315:
1148:
821:
815:
791:
785:
99:+40° 05′ 56.5896″
16:Solar analog star in the constellation Auriga
1809:
1807:
1538:
1066:
2035:
1719:Australia Telescope, Outreach and Education
1660:
1544:
1379:
1257:
1160:The Astrophysical Journal Supplement Series
1095:
994:
725:This star may have been called by the name
2028:
2014:
1916:
1849:
1777:
1740:
1654:
1204:
969:
967:
965:
963:
2744:
1804:
1783:
1768:
1674:
1621:
1560:
1436:
1407:
1362:
1344:
1282:
1224:
1171:
1115:
1023:
942:
932:
922:
891:
889:
887:
885:
883:
881:
879:
608:. It is visible to the naked eye with an
59:J2000
1946:"Combined apparent magnitude of 2 stars"
2949:
1938:
1069:Astrophysical Journal Supplement Series
960:
616:measurements, it is approximately 40.7
211:
3021:
1865:, California Institute of Technology:
1855:
1469:
876:
733:in Arabic. Lambda Aurigae, along with
2009:
1856:Rhoads, Jack W. (November 15, 1971),
1813:
1707:
1513:
1213:Astronomy and Astrophysics Supplement
895:
1978:from the original on 1 February 2012
1902:
1725:, December 21, 2004, archived from
663:is showing some features of a more
223:
13:
1821:Star Names: Their Lore and Meaning
14:
3095:
1994:
1749:The Astrophysical Journal Letters
1519:
828:the Third Star of Pool of Harmony
3005:
3004:
1364:10.1111/j.1365-2966.2009.15048.x
246:80.1054 ± 0.2158
37:
30:
1960:
1879:
951:Gaia DR2 record for this source
713:components of this star are =
48:Location of λ Aurigae (circled)
3074:Henry Draper Catalogue objects
833:
1:
3084:Bright Star Catalogue objects
1522:"LAMBDA AUR (Lambda Aurigae)"
869:
646:
1610:Astronomy & Astrophysics
910:Astronomy & Astrophysics
7:
2048:Auriga in Chinese astronomy
1770:10.1088/2041-8205/747/2/L32
1640:10.1051/0004-6361/201833456
1134:10.1051/0004-6361/200811191
1042:10.1088/0004-637X/746/1/101
944:10.1051/0004-6361/201833051
822:
792:
10:
3100:
3029:G-type main-sequence stars
1786:Astronomy and Astrophysics
1579:10.1051/0004-6361:20078357
1548:Astronomy and Astrophysics
1505:: CS1 maint: postscript (
1301:10.1051/0004-6361:20031378
1270:Astronomy and Astrophysics
1104:Astronomy and Astrophysics
3002:
2976:
2945:
2915:
2894:
2885:
2850:
2807:
2796:
2740:
2690:
2647:
2559:
2426:
2246:
2070:
2061:
2043:
1867:Jet Propulsion Laboratory
1425:The Astrophysical Journal
1012:The Astrophysical Journal
827:
816:
786:
703:Epsilon Indi Moving Group
653:G-type main sequence star
610:apparent visual magnitude
549:
492:
485:
481:
300:
295:
291:
174:
167:
116:
53:
24:
1663:The Astronomical Journal
842:, Lambda Aurigae has an
814:for λ Aurigae itself is
2053:List of stars in Auriga
2037:Constellation of Auriga
1798:1978A&A....68...27K
1632:2018A&A...616A..37B
1571:2007A&A...474..653V
1293:2003A&A...411..559K
1235:2000A&AS..141..491C
1126:2009A&A...501..941H
934:2018A&A...616A...1G
720:
589:from λ Aurigae, is the
277:Absolute magnitude
106:Apparent magnitude
3059:Durchmusterung objects
1968:"Magnitude Arithmetic"
705:of stars that share a
657:stellar classification
3069:Gliese and GJ objects
2677:45350 (Lucilinburhuc)
1715:"The Colour of Stars"
1594:see VizieR catalogue
680:effective temperature
2001:Image Lambda Aurigae
1409:10.1093/pasj/57.1.13
810:. Consequently, the
612:of 4.71. Based upon
226: −664.826
214: +520.581
1761:2012ApJ...747L..32L
1685:2005AJ....129.1483L
1447:2008ApJ...687.1264M
1400:2005PASJ...57...13T
1355:2009MNRAS.397..757G
1243:10.1051/aas:2000124
1182:2007ApJS..168..297T
1081:1989ApJS...71..245K
1034:2012ApJ...746..101B
988:1966CoLPL...4...99J
709:through space. The
550:Database references
448:Rotational velocity
266:(12.48 ± 0.03
21:
844:apparent magnitude
487:Other designations
123:Spectral type
19:
3079:Hipparcos objects
3064:Flamsteed objects
3016:
3015:
2998:
2997:
2990:MACS J0717.5+3745
2972:
2971:
2941:
2940:
2881:
2880:
2792:
2791:
2736:
2735:
1897:978-986-7332-25-7
1836:978-0-486-21079-7
1729:on March 18, 2012
741:, were Kazwini's
632:, traversing the
591:Bayer designation
580:
579:
3091:
3039:Solar-type stars
3034:G-type subgiants
3008:
3007:
2978:
2977:
2947:
2946:
2933:Westbrook Nebula
2892:
2891:
2805:
2804:
2742:
2741:
2068:
2067:
2030:
2023:
2016:
2007:
2006:
1988:
1987:
1985:
1983:
1964:
1958:
1957:
1955:
1953:
1942:
1936:
1935:
1933:
1931:
1920:
1914:
1910:
1906:
1900:
1887:
1883:
1877:
1876:
1874:
1873:
1864:
1853:
1847:
1846:
1844:
1843:
1824:
1811:
1802:
1801:
1781:
1775:
1774:
1772:
1744:
1738:
1737:
1735:
1734:
1711:
1705:
1704:
1678:
1676:astro-ph/0412070
1669:(3): 1483–1522,
1658:
1652:
1651:
1625:
1605:
1599:
1590:
1564:
1542:
1536:
1535:
1533:
1532:
1517:
1511:
1510:
1504:
1496:
1494:
1493:
1473:
1467:
1466:
1440:
1431:(2): 1264–1293,
1420:
1414:
1413:
1411:
1383:
1377:
1376:
1366:
1348:
1326:
1313:
1312:
1286:
1284:astro-ph/0308429
1264:
1255:
1254:
1228:
1226:astro-ph/9912342
1208:
1202:
1201:
1175:
1173:astro-ph/0607235
1155:
1146:
1145:
1119:
1099:
1093:
1092:
1064:
1055:
1053:
1027:
1007:
992:
991:
971:
958:
948:
946:
936:
926:
893:
829:
825:
819:
818:
795:
789:
788:
716:
685:
676:outer atmosphere
642:
634:celestial sphere
600:in the northern
507:
474:4, 5.0–7.9
422:
420:
375:
373:
348:
346:
321:
320:
319:
261:40.7 ± 0.1
225:
213:
197:
195:
130:
117:Characteristics
109:
89:
84:
54:Observation data
41:
34:
22:
18:
3099:
3098:
3094:
3093:
3092:
3090:
3089:
3088:
3044:Maunder Minimum
3019:
3018:
3017:
3012:
2994:
2982:Galaxy clusters
2968:
2937:
2911:
2877:
2846:
2799:
2788:
2754:HAT-P-9b (Alef)
2732:
2723:UGPS J0521+3640
2703:HAT-P-9 (Tevel)
2686:
2643:
2555:
2422:
2242:
2057:
2039:
2034:
1997:
1992:
1991:
1981:
1979:
1966:
1965:
1961:
1951:
1949:
1944:
1943:
1939:
1929:
1927:
1922:
1921:
1917:
1908:
1907:
1903:
1885:
1884:
1880:
1871:
1869:
1862:
1854:
1850:
1841:
1839:
1837:
1812:
1805:
1782:
1778:
1745:
1741:
1732:
1730:
1713:
1712:
1708:
1659:
1655:
1606:
1602:
1543:
1539:
1530:
1528:
1518:
1514:
1498:
1497:
1491:
1489:
1475:
1474:
1470:
1421:
1417:
1384:
1380:
1327:
1316:
1265:
1258:
1209:
1205:
1156:
1149:
1100:
1096:
1065:
1058:
1054:. See Table 10.
1008:
995:
972:
961:
897:Brown, A. G. A.
894:
877:
872:
836:
799:Pool of Harmony
723:
714:
692:Maunder minimum
683:
649:
637:
636:at the rate of
626:radial velocity
545:
502:
499:15 Aurigae
454: sin
418:
416:
391:Surface gravity
383:
380:
371:
369:
356:
353:
344:
342:
329:
326:
317:
315:
314:
312:
282:
265:
222:
193:
191:
186:
181:Radial velocity
128:
104:
87:
82:Right ascension
80:
55:
49:
47:
46:
45:
44:
43:
42:
17:
12:
11:
5:
3097:
3087:
3086:
3081:
3076:
3071:
3066:
3061:
3056:
3051:
3046:
3041:
3036:
3031:
3014:
3013:
3003:
3000:
2999:
2996:
2995:
2993:
2992:
2986:
2984:
2974:
2973:
2970:
2969:
2967:
2966:
2961:
2955:
2953:
2943:
2942:
2939:
2938:
2936:
2935:
2930:
2925:
2919:
2917:
2913:
2912:
2910:
2909:
2904:
2898:
2896:
2889:
2883:
2882:
2879:
2878:
2876:
2875:
2870:
2865:
2860:
2854:
2852:
2848:
2847:
2845:
2844:
2839:
2834:
2829:
2824:
2819:
2813:
2811:
2802:
2794:
2793:
2790:
2789:
2787:
2786:
2781:
2776:
2771:
2766:
2761:
2756:
2750:
2748:
2738:
2737:
2734:
2733:
2731:
2730:
2725:
2720:
2715:
2710:
2705:
2700:
2694:
2692:
2688:
2687:
2685:
2684:
2682:49674 (Nervia)
2679:
2674:
2669:
2664:
2659:
2653:
2651:
2645:
2644:
2642:
2641:
2636:
2631:
2626:
2621:
2616:
2611:
2606:
2601:
2596:
2591:
2586:
2581:
2576:
2571:
2565:
2563:
2557:
2556:
2554:
2553:
2548:
2543:
2538:
2533:
2528:
2523:
2518:
2513:
2508:
2503:
2498:
2493:
2488:
2483:
2478:
2473:
2468:
2463:
2458:
2453:
2448:
2443:
2438:
2432:
2430:
2424:
2423:
2421:
2420:
2413:
2408:
2403:
2398:
2393:
2388:
2383:
2378:
2373:
2368:
2363:
2358:
2353:
2348:
2343:
2338:
2333:
2328:
2323:
2318:
2313:
2308:
2303:
2298:
2293:
2288:
2283:
2278:
2273:
2268:
2263:
2258:
2252:
2250:
2244:
2243:
2241:
2240:
2235:
2230:
2225:
2220:
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2145:
2140:
2135:
2127:
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2107:
2102:
2097:
2092:
2087:
2085:β (Menkalinan)
2082:
2076:
2074:
2065:
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2018:
2010:
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1996:
1995:External links
1993:
1990:
1989:
1959:
1948:. WolframΑlpha
1937:
1915:
1901:
1878:
1848:
1835:
1803:
1792:(1–2): 27–31,
1776:
1739:
1706:
1693:10.1086/427854
1653:
1600:
1555:(2): 653–664,
1537:
1520:Kaler, James,
1512:
1468:
1455:10.1086/591785
1415:
1378:
1339:(2): 757–762,
1314:
1277:(3): 559–564,
1256:
1219:(3): 491–506,
1203:
1190:10.1086/509763
1166:(2): 297–318,
1147:
1110:(3): 941–947,
1094:
1089:10.1086/191373
1056:
993:
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874:
873:
871:
868:
850:, located 4.5
835:
832:
722:
719:
711:space velocity
648:
645:
583:Lambda Aurigae
578:
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506:+39° 1248
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88:05 19 08.47546
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3054:Bayer objects
3052:
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2718:SGR 0501+4516
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2105:ζ (Saclateni)
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707:common motion
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668:subgiant star
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630:proper motion
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229:
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210:
208:
206:
205:Proper motion
202:
201:
190:
188:
182:
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177:
173:
170:
166:
162:
160:
156:
155:
151:
149:
145:
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134:
133:
127:G1 V or
126:
124:
121:
120:
115:
111:
107:
103:
102:
98:
96:
93:
92:
86:
83:
79:
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72:
70:
69:Constellation
67:
66:
62:
58:
52:
40:
33:
23:
2415:
2131:
2129:
2120:ι (Hassaleh)
1980:. Retrieved
1972:Weekly Topic
1971:
1962:
1950:. Retrieved
1940:
1928:. Retrieved
1926:. SolStation
1918:
1909:(in Chinese)
1904:
1888:
1886:(in Chinese)
1881:
1870:, retrieved
1858:
1851:
1840:. Retrieved
1820:
1815:Allen, R. H.
1789:
1785:
1779:
1752:
1748:
1742:
1731:, retrieved
1727:the original
1718:
1709:
1666:
1662:
1656:
1613:
1609:
1603:
1591:
1552:
1546:
1540:
1529:, retrieved
1525:
1515:
1490:. Retrieved
1480:
1471:
1428:
1424:
1418:
1394:(1): 13–25,
1391:
1387:
1381:
1336:
1330:
1274:
1268:
1216:
1212:
1206:
1163:
1159:
1107:
1103:
1097:
1072:
1068:
1015:
1011:
979:
975:
914:
908:
902:
837:
823:Xián Chí sān
812:Chinese name
797:
779:
775:Al Ḣibāʽ III
774:
766:
758:
754:
750:
746:
742:
730:
726:
724:
699:disk of dust
696:
650:
595:solar analog
582:
581:
569:
555:
544: 11625
540: 1753,
528: 1729,
512: 1145,
467:
455:
451:
446:
431:
409:
394:
389:
362:
335:
305:
275:
254:
238:
203:
179:
2115:θ (Mahasim)
2080:α (Capella)
1982:10 February
1952:10 February
1930:10 February
1924:"Capella 4"
1562:0708.1752v1
860:star system
852:light-years
834:Observation
826:, English:
796:), meaning
767:Al Ḣibāʽ II
688:G-type star
684:5890 K
618:light-years
536: 403,
516: 197,
462:2 km/s
438:+0.12
433:Metallicity
411:Temperature
159:color index
148:color index
137:color index
95:Declination
3023:Categories
2868:Messier 38
2863:Messier 37
2858:Messier 36
2774:HD 49674 b
2769:HD 45350 b
2764:HD 43691 b
2759:HD 40979 b
2746:Exoplanets
2698:Gliese 268
2110:η (Haedus)
2100:ε (Almaaz)
2090:γ (Elnath)
1974:. Caglow.
1872:2012-08-19
1842:2010-12-12
1755:(2): L32,
1733:2012-01-16
1623:1805.07581
1531:2011-12-11
1492:2012-08-19
1018:(1): 101,
982:(99): 99,
924:1804.09365
870:References
759:Al Ḣibāʽ I
729:, meaning
651:This is a
647:Properties
643:per year.
401:4.02
393:(log
364:Luminosity
198: km/s
169:Astrometry
20:λ Aurigae
2964:4C +41.17
2873:Palomar 2
2248:Flamsteed
1477:"lam Aur"
1438:0807.1686
1346:0907.3677
1142:118577511
1117:0811.3982
1025:1112.3316
804:ρ Aurigae
587:Latinized
108: (V)
3010:Category
2951:Galaxies
2800:clusters
2784:WASP-12b
2779:KELT-2Ab
2428:Variable
2132:(Alhurr)
1976:Archived
1817:(1963).
1648:56269929
1587:18759600
1501:cite web
1463:27151456
1373:17758971
1309:18478960
1251:16273589
1198:18775378
1050:18993744
808:HD 36041
793:Xián Chí
755:Al Ḣibāʽ
743:Al Ḣibāʽ
731:the fawn
694:analog.
661:spectrum
614:parallax
382:☉
355:☉
328:☉
279: (M
256:Distance
240:Parallax
2928:IC 2149
2887:Nebulae
2728:WASP-12
2713:MWC 480
2481:AR (17)
2446:RT (48)
1794:Bibcode
1757:Bibcode
1701:2603568
1681:Bibcode
1628:Bibcode
1616:: A37,
1567:Bibcode
1443:Bibcode
1396:Bibcode
1351:Bibcode
1289:Bibcode
1231:Bibcode
1178:Bibcode
1122:Bibcode
1077:Bibcode
1075:: 245,
1030:Bibcode
984:Bibcode
929:Bibcode
856:parsecs
848:Capella
782:Chinese
727:Al Hurr
665:evolved
655:with a
622:parsecs
296:Details
61:Equinox
3049:Auriga
2959:3C 147
2923:IC 405
2708:KELT-2
2417:35 Cam
1895:
1889:中國星座神話
1833:
1699:
1646:
1585:
1482:SIMBAD
1461:
1371:
1307:
1249:
1196:
1140:
1048:
955:VizieR
917:. A1.
864:Sirius
747:ألحباع
678:at an
620:(12.5
606:Auriga
593:for a
570:ARICNS
557:SIMBAD
423:
376:
349:
337:Radius
322:
318:−0.029
316:+0.054
192:+66.53
152:+0.62
141:+0.13
74:Auriga
63:J2000
2916:Other
2851:Other
2691:Other
2672:43691
2667:35619
2662:33463
2657:33203
2072:Bayer
2063:Stars
1863:(PDF)
1697:S2CID
1671:arXiv
1644:S2CID
1618:arXiv
1596:I/311
1592:Note:
1583:S2CID
1557:arXiv
1526:Stars
1459:S2CID
1433:arXiv
1369:S2CID
1341:arXiv
1305:S2CID
1279:arXiv
1247:S2CID
1221:arXiv
1194:S2CID
1168:arXiv
1138:S2CID
1112:arXiv
1046:S2CID
1020:arXiv
949:
919:arXiv
854:(1.4
840:Earth
838:From
771:σ Aur
763:μ Aur
739:σ Aur
735:μ Aur
638:0.844
495:λ Aur
417:5,890
374:0.022
370:1.732
347:0.021
343:1.331
313:1.081
224:Dec.:
163:0.32
112:4.71
57:Epoch
2907:2242
2902:1985
2842:2281
2837:2240
2832:1931
2827:1907
2822:1893
2817:1664
2798:Star
2639:2137
2634:2096
2629:2028
2624:1945
2619:1938
2614:1884
2609:1866
2604:1825
2599:1822
2594:1795
2589:1794
2584:1752
2579:1738
2574:1615
2569:1558
2551:V538
2546:V433
2541:V420
2536:V394
2531:V361
2526:V352
1984:2023
1954:2023
1932:2023
1893:ISBN
1831:ISBN
1507:link
903:Gaia
806:and
769:and
737:and
721:Name
715:km/s
598:star
575:data
563:data
307:Mass
287:4.20
196:0.14
157:R−I
146:B−V
135:U−B
2895:NGC
2809:NGC
1765:doi
1753:747
1689:doi
1667:129
1636:doi
1614:616
1575:doi
1553:474
1451:doi
1429:687
1404:doi
1359:doi
1337:397
1297:doi
1275:411
1239:doi
1217:141
1186:doi
1164:168
1130:doi
1108:501
1085:doi
1038:doi
1016:746
953:at
939:doi
915:616
830:.)
817:咸池三
780:In
773:as
765:as
682:of
672:Sun
604:of
542:LTT
538:LHS
534:LFT
530:SAO
522:HIP
510:FK5
476:Gyr
469:Age
440:dex
421:4.3
403:cgs
248:mas
242:(π)
228:mas
216:mas
212:RA:
207:(μ)
3025::
2649:HD
2561:HR
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