31:
2399:
589:
1108:
Arroyo-Torres, B.; Wittkowski, M.; Chiavassa, A.; Scholz, M.; Freytag, B.; Marcaide, J. M.; Hauschildt, P. H.; Wood, P. R.; Abellan, F. J. (2015). "What causes the large extensions of red supergiant atmospheres?. Comparisons of interferometric observations with 1D hydrostatic, 3D convection, and 1D
1055:; Massey, Philip; Olsen, K. A. G.; Plez, Bertrand; Josselin, Eric; Maeder, Andre; Meynet, Georges (2005). "The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool as We Thought".
585:
per year. An excess of emission at long wavelengths from this star, as well as a small amount of silicate emission, suggests that it may be enclosed by an extensive cloud of dust.
607:
with a maximum brightness range of magnitude 7.6 - 9.1 and a period of 635 or 672 days. Despite the large amplitude of variation, it was only named as a variable star in 2006.
2431:
1308:
352:
1005:"The effect of winds on atmospheric layers of red supergiants II. Modelling VLTI/GRAVITY and MATISSE observations of AH Sco, KW Sgr, V602 Car, CK Car and V460 Car"
882:
Melnik, A. M.; Dambis, A. K. (2020). "Distance scale for high-luminosity stars in OB associations and in field with Gaia DR2. Spurious systematic motions".
57:
2436:
1221:
Humphreys, Roberta M.; Strecker, Donald W.; Ney, E. P. (February 1972), "Spectroscopic and
Photometric Observations of M Supergiants in Carina",
644:
Hog, E.; Kuzmin, A.; Bastian, U.; Fabricius, C.; Kuimov, K.; Lindegren, L.; Makarov, V. V.; Roeser, S. (1998). "The TYCHO Reference
Catalogue".
1301:
736:
Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data
Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)".
2441:
1263:
Kazarovets, E. V.; Samus, N. N.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (2006). "The 78th Name-List of
Variable Stars".
2456:
2446:
2426:
2402:
1294:
50:
2325:
2369:
2461:
2421:
1333:
455:
1870:
824:
676:
Mauron, N.; Josselin, E. (February 2011), "The mass-loss rates of red supergiants and the de Jager prescription",
1410:
811:
604:
386:
159:
20:
1860:
865:
763:
Keenan, Philip C.; McNeil, Raymond C. (1989). "The
Perkins catalog of revised MK types for the cooler stars".
559:
based on the same effective temperature derived in 2005. The radius was measured again in 2024 at 1,015
1328:
2451:
1796:
1317:
451:
394:
390:
122:
70:
2245:
2061:
1633:
480:
360:
1272:
1230:
1185:
1128:
1074:
954:
901:
843:
772:
745:
695:
653:
229:
2275:
531:
1865:
1203:
1175:
1144:
1118:
1090:
1064:
1016:
970:
944:
917:
891:
833:
788:
711:
685:
593:
423:
250:
102:
2260:
1352:
1034:
43:
1238:
1193:
1136:
1132:
1082:
1026:
962:
909:
905:
853:
848:
780:
703:
699:
657:
462:
327:
213:
1390:
1370:
340:
78:
30:
530:
was then calculated from the luminosity and radius. A more recent measurement based on a
1276:
1234:
1189:
1164:"A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2"
1078:
958:
776:
749:
2351:
2343:
1880:
1875:
1052:
541:
439:
378:
221:
201:
189:
2415:
2240:
2125:
1400:
1380:
1207:
974:
921:
792:
715:
447:
443:
178:
154:
65:
1148:
1094:
461:
In 2005, V602 Car was calculated to have a bolometric luminosity below 110,000
2160:
2050:
2011:
2006:
2001:
1996:
1991:
1986:
1623:
1578:
1573:
1568:
1563:
1558:
1548:
1543:
1538:
1533:
1523:
1518:
1513:
1508:
1498:
1385:
1365:
522:
based on the measured angular diameter and luminosity. An effective temperature of
471:
307:
280:
1140:
1030:
858:
815:
707:
738:
VizieR On-line Data
Catalog: B/GCVS. Originally Published in: 2009yCat....102025S
2382:
2155:
2150:
2145:
2031:
1915:
1910:
1905:
1890:
1618:
1613:
1608:
1603:
1598:
1395:
1375:
596:
588:
144:
133:
91:
1198:
1163:
913:
2377:
2250:
2120:
2115:
2036:
2026:
2021:
2016:
1900:
1895:
1493:
1488:
1483:
1478:
1473:
1468:
1463:
1458:
1453:
1448:
1443:
966:
621:
616:
576:
320:
287:
236:
166:
1038:
1003:
González-Torà, G.; Wittkowski, M.; Davies, B.; Plez, B. (December 19, 2023).
2140:
1978:
1641:
1438:
1428:
1418:
508:
based on the measured flux and an assumed distance, and a larger radius of
1286:
2309:
2255:
2224:
2219:
2214:
2209:
2204:
2199:
2194:
2189:
2099:
2094:
2089:
2084:
2079:
2074:
2069:
1844:
1839:
1834:
1829:
1824:
1819:
1814:
1809:
1804:
1786:
1781:
1776:
1771:
1761:
1756:
1751:
1741:
1731:
1726:
1721:
1716:
1711:
1706:
1701:
1696:
1691:
1681:
1676:
1671:
1666:
1661:
1646:
1593:
1583:
1528:
1503:
1433:
1423:
1069:
2270:
2265:
2135:
2130:
1920:
1885:
1766:
1746:
1736:
1686:
1656:
1651:
1553:
1360:
53:
46:
2294:
2280:
2174:
1960:
1955:
1950:
1930:
1925:
869:
486:
417:
367:
300:
241:
1243:
1180:
1123:
1086:
1021:
935:
Fadeyev, Yu. A. (2012). "Nonlinear pulsations of red supergiants".
896:
838:
784:
1945:
1940:
1935:
1004:
949:
690:
587:
490:. A 2015 study derived a slightly higher bolometric luminosity of
402:
1343:
398:
205:
193:
1290:
820:
Data
Release 2: Summary of the contents and survey properties"
2368:
2342:
2318:
2302:
2293:
2233:
2182:
2173:
2108:
2060:
2049:
1977:
1853:
1795:
1632:
1409:
1351:
1342:
814:; et al. (Gaia collaboration) (August 2018).
458:, being around 1,000 times larger than the Sun.
998:
996:
994:
992:
990:
988:
986:
984:
1302:
671:
669:
667:
8:
569:V602 Car has an estimated mass loss rate of
96:−60° 05′ 28.838″
545:gives a luminosity at 125,000–131,000
2365:
2339:
2299:
2179:
2057:
1974:
1348:
1309:
1295:
1287:
1242:
1197:
1179:
1122:
1068:
1020:
948:
895:
857:
847:
837:
689:
599:for V602 Carinae, plotted from AAVSO data
552:with a corresponding radius of 932
2432:Objects with variable star designations
1258:
1256:
1254:
765:Astrophysical Journal Supplement Series
639:
637:
633:
185:
1265:Information Bulletin on Variable Stars
1162:Messineo, M.; Brown, A. G. A. (2019).
731:
729:
727:
725:
18:
806:
804:
802:
7:
49:
197:
14:
2398:
2397:
29:
16:Star in the constellation Carina
866:Gaia DR2 record for this source
220:0.4366 ± 0.0698
2437:Henry Draper Catalogue objects
2326:Carina Dwarf Spheroidal Galaxy
1109:pulsating model atmospheres".
884:Astrophysics and Space Science
479:based on the assumption of an
389: Carinae, V602 Car,
286:17.7 – 20
1:
470:and a radius around 860
1111:Astronomy & Astrophysics
1009:Astronomy & Astrophysics
825:Astronomy & Astrophysics
1334:Carina in Chinese astronomy
1141:10.1051/0004-6361/201425212
1031:10.1051/0004-6361/202348047
859:10.1051/0004-6361/201833051
708:10.1051/0004-6361/201013993
2478:
2442:Semiregular variable stars
914:10.1007/s10509-020-03827-0
678:Astronomy and Astrophysics
646:Astronomy and Astrophysics
456:one of largest known stars
2395:
2364:
2338:
1973:
1324:
1057:The Astrophysical Journal
967:10.1134/S1063773712040032
605:semiregular variable star
454:. It is considered to be
410:
384:
377:
373:
274:
269:
265:
172:
165:
116:
40:
27:
1199:10.3847/1538-3881/ab1cbd
1168:The Astronomical Journal
450:M3 in the constellation
405: J11132996-6005288
188: −5.425
1329:List of stars in Carina
1318:Constellation of Carina
1133:2015A&A...575A..50A
906:2020Ap&SS.365..112M
849:2018A&A...616A...1G
700:2011A&A...526A.156M
658:1998A&A...335L..65H
251:Absolute magnitude
103:Apparent magnitude
2457:IRAS catalogue objects
2447:Durchmusterung objects
2427:Carina (constellation)
600:
2246:Finger of God Globule
2037:HD 95086 b (Levantes)
1223:Astrophysical Journal
591:
481:effective temperature
240:(approx. 2,300
35:Location of V602 Car
2370:Astronomical events
1277:2006IBVS.5721....1K
1235:1972ApJ...172...75H
1190:2019AJ....158...20M
1079:2005ApJ...628..973L
959:2012AstL...38..260F
777:1989ApJS...71..245K
750:2009yCat....102025S
532:Gaia Data Release 2
411:Database references
235:approx. 7,000
24:
2462:Population I stars
2422:M-type supergiants
2017:HD 63765 b (Yvaga)
1053:Levesque, Emily M.
601:
436:V602 Car, HD 97671
401: 11113-5949,
379:Other designations
155:Variable type
123:Spectral type
19:
2409:
2408:
2391:
2390:
2360:
2359:
2334:
2333:
2289:
2288:
2261:Homunculus Nebula
2169:
2168:
2045:
2044:
1969:
1968:
937:Astronomy Letters
429:
428:
200: 2.183
2469:
2401:
2400:
2366:
2340:
2300:
2180:
2058:
1975:
1429:T (not variable)
1349:
1311:
1304:
1297:
1288:
1281:
1280:
1260:
1249:
1248:
1246:
1218:
1212:
1211:
1201:
1183:
1159:
1153:
1152:
1126:
1105:
1099:
1098:
1072:
1070:astro-ph/0504337
1049:
1043:
1042:
1024:
1000:
979:
978:
952:
932:
926:
925:
899:
879:
873:
863:
861:
851:
841:
808:
797:
796:
760:
754:
753:
733:
720:
719:
693:
673:
662:
661:
641:
584:
574:
544:
539:
529:
527:
521:
513:
507:
499:
498:
489:
397:−59°3623,
261:–4.83 (variable)
199:
187:
117:Characteristics
112:
106:
86:
81:
41:Observation data
33:
25:
2477:
2476:
2472:
2471:
2470:
2468:
2467:
2466:
2412:
2411:
2410:
2405:
2387:
2356:
2344:Galaxy clusters
2330:
2314:
2285:
2276:IGR J11014−6103
2229:
2165:
2104:
2052:
2041:
1965:
1849:
1810:63765 (Tapecue)
1791:
1628:
1405:
1366:β (Miaplacidus)
1338:
1320:
1315:
1285:
1284:
1262:
1261:
1252:
1220:
1219:
1215:
1161:
1160:
1156:
1107:
1106:
1102:
1051:
1050:
1046:
1002:
1001:
982:
934:
933:
929:
881:
880:
876:
812:Brown, A. G. A.
810:
809:
800:
762:
761:
757:
735:
734:
723:
675:
674:
665:
643:
642:
635:
630:
613:
582:
572:
570:
565:
562:
558:
555:
551:
548:
537:
535:
525:
523:
520:
517:
511:
509:
506:
503:
496:
494:
493:
491:
484:
477:
474:
468:
465:
406:
341:Surface gravity
333:
330:
313:
310:
293:
290:
256:
239:
196:
110:
101:
84:
79:Right ascension
77:
42:
36:
34:
17:
12:
11:
5:
2475:
2473:
2465:
2464:
2459:
2454:
2449:
2444:
2439:
2434:
2429:
2424:
2414:
2413:
2407:
2406:
2396:
2393:
2392:
2389:
2388:
2386:
2385:
2380:
2374:
2372:
2362:
2361:
2358:
2357:
2355:
2354:
2352:Bullet Cluster
2348:
2346:
2336:
2335:
2332:
2331:
2329:
2328:
2322:
2320:
2316:
2315:
2313:
2312:
2306:
2304:
2297:
2291:
2290:
2287:
2286:
2284:
2283:
2278:
2273:
2268:
2263:
2258:
2253:
2248:
2243:
2237:
2235:
2231:
2230:
2228:
2227:
2222:
2217:
2212:
2207:
2202:
2197:
2192:
2186:
2184:
2177:
2171:
2170:
2167:
2166:
2164:
2163:
2158:
2153:
2148:
2143:
2138:
2133:
2128:
2123:
2118:
2112:
2110:
2106:
2105:
2103:
2102:
2097:
2092:
2087:
2082:
2077:
2072:
2066:
2064:
2055:
2047:
2046:
2043:
2042:
2040:
2039:
2034:
2029:
2024:
2019:
2014:
2009:
2004:
1999:
1994:
1989:
1983:
1981:
1971:
1970:
1967:
1966:
1964:
1963:
1958:
1953:
1948:
1943:
1938:
1933:
1928:
1923:
1918:
1913:
1908:
1903:
1898:
1893:
1888:
1883:
1878:
1873:
1868:
1863:
1857:
1855:
1851:
1850:
1848:
1847:
1842:
1837:
1832:
1827:
1822:
1817:
1812:
1807:
1801:
1799:
1793:
1792:
1790:
1789:
1784:
1779:
1774:
1769:
1764:
1759:
1754:
1749:
1744:
1739:
1734:
1729:
1724:
1719:
1714:
1709:
1704:
1699:
1694:
1689:
1684:
1679:
1674:
1669:
1664:
1659:
1654:
1649:
1644:
1638:
1636:
1630:
1629:
1627:
1626:
1621:
1616:
1611:
1606:
1601:
1596:
1591:
1586:
1581:
1576:
1571:
1566:
1561:
1556:
1551:
1546:
1541:
1536:
1531:
1526:
1521:
1516:
1511:
1506:
1501:
1496:
1491:
1486:
1481:
1476:
1471:
1466:
1461:
1456:
1451:
1446:
1441:
1436:
1431:
1426:
1421:
1415:
1413:
1407:
1406:
1404:
1403:
1398:
1393:
1388:
1383:
1378:
1373:
1368:
1363:
1357:
1355:
1346:
1340:
1339:
1337:
1336:
1331:
1325:
1322:
1321:
1316:
1314:
1313:
1306:
1299:
1291:
1283:
1282:
1250:
1244:10.1086/151329
1213:
1154:
1100:
1087:10.1086/430901
1063:(2): 973–985.
1044:
980:
943:(4): 260–270.
927:
874:
798:
785:10.1086/191373
755:
721:
663:
632:
631:
629:
626:
625:
624:
619:
612:
609:
603:V602 Car is a
580:
563:
560:
556:
553:
549:
546:
518:
515:
504:
501:
475:
472:
466:
463:
440:red supergiant
427:
426:
421:
413:
412:
408:
407:
385:
382:
381:
375:
374:
371:
370:
364:
356:
355:
349:
336:
335:
331:
328:
324:
316:
315:
311:
308:
304:
296:
295:
291:
288:
284:
276:
275:
272:
271:
267:
266:
263:
262:
259:
254:
246:
245:
233:
225:
224:
218:
209:
208:
183:
174:
173:
170:
169:
163:
162:
157:
151:
150:
147:
140:
139:
136:
129:
128:
125:
119:
118:
114:
113:
107:
98:
97:
94:
88:
87:
82:
74:
73:
68:
62:
61:
38:
37:
28:
15:
13:
10:
9:
6:
4:
3:
2:
2474:
2463:
2460:
2458:
2455:
2453:
2452:2MASS objects
2450:
2448:
2445:
2443:
2440:
2438:
2435:
2433:
2430:
2428:
2425:
2423:
2420:
2419:
2417:
2404:
2394:
2384:
2381:
2379:
2376:
2375:
2373:
2371:
2367:
2363:
2353:
2350:
2349:
2347:
2345:
2341:
2337:
2327:
2324:
2323:
2321:
2317:
2311:
2308:
2307:
2305:
2301:
2298:
2296:
2292:
2282:
2279:
2277:
2274:
2272:
2269:
2267:
2264:
2262:
2259:
2257:
2254:
2252:
2249:
2247:
2244:
2242:
2241:Carina Nebula
2239:
2238:
2236:
2232:
2226:
2223:
2221:
2218:
2216:
2213:
2211:
2208:
2206:
2203:
2201:
2198:
2196:
2193:
2191:
2188:
2187:
2185:
2181:
2178:
2176:
2172:
2162:
2159:
2157:
2154:
2152:
2149:
2147:
2144:
2142:
2139:
2137:
2134:
2132:
2129:
2127:
2126:Collinder 228
2124:
2122:
2119:
2117:
2114:
2113:
2111:
2107:
2101:
2098:
2096:
2093:
2091:
2088:
2086:
2083:
2081:
2078:
2076:
2073:
2071:
2068:
2067:
2065:
2063:
2059:
2056:
2054:
2048:
2038:
2035:
2033:
2030:
2028:
2025:
2023:
2020:
2018:
2015:
2013:
2010:
2008:
2005:
2003:
2000:
1998:
1995:
1993:
1990:
1988:
1985:
1984:
1982:
1980:
1976:
1972:
1962:
1959:
1957:
1954:
1952:
1949:
1947:
1944:
1942:
1939:
1937:
1934:
1932:
1929:
1927:
1924:
1922:
1919:
1917:
1914:
1912:
1909:
1907:
1904:
1902:
1899:
1897:
1894:
1892:
1889:
1887:
1884:
1882:
1879:
1877:
1874:
1872:
1871:DEN 0817−6155
1869:
1867:
1864:
1862:
1859:
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1800:
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1597:
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1417:
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1414:
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1408:
1402:
1399:
1397:
1394:
1392:
1389:
1387:
1386:ι (Aspidiske)
1384:
1382:
1379:
1377:
1374:
1372:
1369:
1367:
1364:
1362:
1359:
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1200:
1195:
1191:
1187:
1182:
1177:
1173:
1169:
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1158:
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1146:
1142:
1138:
1134:
1130:
1125:
1120:
1116:
1112:
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1101:
1096:
1092:
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1080:
1076:
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1028:
1023:
1018:
1014:
1010:
1006:
999:
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993:
991:
989:
987:
985:
981:
976:
972:
968:
964:
960:
956:
951:
946:
942:
938:
931:
928:
923:
919:
915:
911:
907:
903:
898:
893:
889:
885:
878:
875:
871:
867:
860:
855:
850:
845:
840:
835:
831:
827:
826:
821:
819:
813:
807:
805:
803:
799:
794:
790:
786:
782:
778:
774:
770:
766:
759:
756:
751:
747:
743:
739:
732:
730:
728:
726:
722:
717:
713:
709:
705:
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697:
692:
687:
683:
679:
672:
670:
668:
664:
659:
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651:
647:
640:
638:
634:
627:
623:
620:
618:
615:
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598:
595:
590:
586:
583:
579:
567:
543:
533:
488:
482:
478:
469:
459:
457:
453:
449:
448:spectral type
445:
444:variable star
441:
437:
433:
425:
422:
420:
419:
415:
414:
409:
404:
400:
396:
393: 97671,
392:
388:
383:
380:
376:
372:
369:
365:
363:
362:
358:
357:
354:
350:
348:
346:
342:
338:
337:
334:
326:126,000
325:
323:
322:
318:
317:
314:
305:
303:
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298:
297:
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285:
283:
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278:
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268:
264:
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223:
219:
217:
215:
211:
210:
207:
203:
195:
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184:
182:
180:
179:Proper motion
176:
175:
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158:
156:
153:
152:
148:
146:
142:
141:
137:
135:
131:
130:
126:
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121:
120:
115:
108:
104:
100:
99:
95:
93:
90:
89:
85:11 13 29.9740
83:
80:
76:
75:
72:
69:
67:
66:Constellation
64:
63:
59:
55:
52:
48:
45:
39:
32:
26:
22:
2161:Westerlund 2
2012:OGLE2-TR-L9b
2007:OGLE-TR-211b
2002:OGLE-TR-182b
1997:OGLE-TR-113b
1992:OGLE-TR-132b
1987:OGLE-TR-111b
1588:
1268:
1264:
1226:
1222:
1216:
1171:
1167:
1157:
1114:
1110:
1103:
1060:
1056:
1047:
1012:
1008:
940:
936:
930:
887:
883:
877:
829:
823:
817:
768:
764:
758:
741:
737:
681:
677:
649:
645:
602:
577:
568:
540:0.0698
534:parallax of
460:
435:
432:V602 Carinae
431:
430:
416:
359:
344:
339:
319:
299:
279:
249:
228:
212:
177:
23:602 Carinae
2383:GRB 080916C
2156:Trumpler 16
2151:Trumpler 15
2146:Trumpler 14
2032:HD 85628 Ab
1916:OGLE2-TR-L9
1911:OGLE-TR-211
1906:OGLE-TR-182
1891:NGC 3603-A1
1881:Innes' star
1866:CPD−57°2874
1361:α (Canopus)
597:light curve
594:visual band
485:3,550
366:3,400
361:Temperature
306:1,015
145:color index
134:color index
111:(7.6 - 9.1)
92:Declination
2416:Categories
2378:GRB 000131
2251:G290.1-0.8
2121:Carina OB2
2116:Carina OB1
2027:HD 65216 c
2022:HD 65216 b
1979:Exoplanets
1901:NGC 3603-C
1896:NGC 3603-B
1876:1E 1048-59
1861:AWI0005x3s
1181:1905.03744
1124:1501.01560
1022:2312.12521
897:2006.14649
890:(7): 112.
839:1804.09365
628:References
622:EV Carinae
617:RT Carinae
528:280 K
351:–0.5
343:(log
321:Luminosity
167:Astrometry
127:M3 Ia-Iab
2141:Platais 8
1371:ε (Avior)
1208:148571616
1174:(1): 20.
1039:0004-6361
975:118612597
950:1112.2365
922:220128144
793:123149047
716:119276502
691:1010.5369
514:165
105: (V)
2403:Category
2295:Galaxies
2256:Hen 2-47
2053:clusters
1787:4325 (z)
1782:4257 (u)
1767:4177 (t)
1762:4164 (t)
1757:4159 (r)
1747:4138 (K)
1742:4114 (s)
1737:4102 (I)
1732:4089 (L)
1727:4025 (M)
1722:3884 (l)
1717:3856 (m)
1712:3825 (h)
1707:3821 (H)
1702:3728 (k)
1697:3696 (g)
1692:3663 (i)
1687:3643 (G)
1682:3598 (b)
1677:3571 (c)
1672:3415 (e)
1667:3414 (e)
1662:3260 (C)
1657:3220 (B)
1652:3159 (D)
1647:2934 (Q)
1642:2435 (N)
1579:V533 (y)
1569:V520 (w)
1559:V448 (O)
1554:V415 (A)
1549:V399 (P)
1544:V382 (x)
1539:V376 (b)
1529:V371 (z)
1524:V357 (a)
1519:V345 (E)
1514:V344 (f)
1509:V343 (d)
1499:V337 (q)
1411:Variable
1149:29210064
1095:15109583
684:: A156,
611:See also
581:☉
575:10
564:☉
557:☉
550:☉
519:☉
505:☉
476:☉
467:☉
332:☉
312:☉
292:☉
253: (M
230:Distance
214:Parallax
2271:IC 2448
2266:IC 2220
2175:Nebulae
2136:IC 2714
2131:IC 2602
1921:Sher 25
1886:LHS 288
1273:Bibcode
1231:Bibcode
1186:Bibcode
1129:Bibcode
1117:: A50.
1075:Bibcode
1015:: A19.
955:Bibcode
902:Bibcode
844:Bibcode
773:Bibcode
771:: 245.
746:Bibcode
696:Bibcode
654:Bibcode
652:: L65.
497:−45,000
495:+66,000
492:138,000
438:) is a
270:Details
54:J2000.0
51:Equinox
47:J2000.0
2281:RCW 49
1961:WR 42e
1956:WR 31a
1951:WR 30a
1931:WR 21a
1926:WR 20a
1489:PP (p)
1229:: 75,
1206:
1147:
1093:
1037:
973:
920:
870:VizieR
832:. A1.
791:
714:
536:0.4366
500:
452:Carina
418:SIMBAD
301:Radius
149:+2.52
138:+2.59
71:Carina
2319:Other
2234:Other
2109:Other
1946:WR 25
1941:WR 24
1936:WR 22
1854:Other
1845:97950
1840:95086
1835:93403
1830:93250
1825:93129
1820:85628
1815:65216
1805:53143
1353:Bayer
1344:Stars
1271:: 1.
1204:S2CID
1176:arXiv
1145:S2CID
1119:arXiv
1091:S2CID
1065:arXiv
1017:arXiv
971:S2CID
945:arXiv
918:S2CID
892:arXiv
864:
834:arXiv
789:S2CID
712:S2CID
686:arXiv
524:3,432
510:1,050
403:2MASS
198:Dec.:
109:8.39
44:Epoch
2310:3059
2225:3586
2220:3584
2215:3582
2210:3581
2205:3579
2200:3576
2195:3199
2190:2867
2100:3603
2095:3532
2090:3324
2085:3293
2080:3114
2075:2808
2070:2516
2051:Star
1777:4222
1772:4205
1752:4142
1624:V906
1619:V817
1614:V816
1609:V759
1604:V752
1599:V742
1594:V640
1589:V602
1584:V560
1574:V528
1564:V518
1534:V372
1504:V341
1269:5721
1035:ISSN
818:Gaia
442:and
424:data
399:IRAS
387:V602
281:Mass
143:B−V
132:U−B
58:ICRS
2303:NGC
2183:NGC
2062:NGC
1239:doi
1227:172
1194:doi
1172:158
1137:doi
1115:575
1083:doi
1061:628
1027:doi
1013:683
963:doi
910:doi
888:365
868:at
854:doi
830:616
781:doi
704:doi
682:526
650:335
542:mas
483:of
446:of
353:cgs
222:mas
216:(π)
202:mas
190:mas
186:RA:
181:(μ)
160:SRc
2418::
1797:HD
1634:HR
1494:QZ
1484:OY
1479:IX
1474:HR
1469:GG
1464:EV
1459:CK
1454:BO
1449:AG
1444:RT
1267:.
1253:^
1237:,
1225:,
1202:.
1192:.
1184:.
1170:.
1166:.
1143:.
1135:.
1127:.
1113:.
1089:.
1081:.
1073:.
1059:.
1033:.
1025:.
1011:.
1007:.
983:^
969:.
961:.
953:.
941:38
939:.
916:.
908:.
900:.
886:.
852:.
842:.
828:.
822:.
801:^
787:.
779:.
769:71
767:.
744:.
740:.
724:^
710:,
702:,
694:,
680:,
666:^
648:.
636:^
592:A
571:10
566:.
395:CD
391:HD
242:pc
237:ly
206:yr
194:yr
60:)
1439:Y
1434:U
1424:S
1419:R
1401:ω
1396:χ
1391:υ
1381:θ
1376:η
1310:e
1303:t
1296:v
1279:.
1275::
1247:.
1241::
1233::
1210:.
1196::
1188::
1178::
1151:.
1139::
1131::
1121::
1097:.
1085::
1077::
1067::
1041:.
1029::
1019::
977:.
965::
957::
947::
924:.
912::
904::
894::
872:.
862:.
856::
846::
836::
816:"
795:.
783::
775::
752:.
748::
742:1
718:.
706::
698::
688::
660:.
656::
578:M
573:×
561:R
554:R
547:L
538:±
526:±
516:R
512:±
502:L
487:K
473:R
464:L
434:(
368:K
347:)
345:g
329:L
309:R
289:M
257:)
255:V
244:)
204:/
192:/
56:(
21:V
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