638:
1946:
1255:. Variable Stars in the Local Group, IAU Colloquium 193, Proceedings of the conference held 6-11 July, 2003 at Christchurch, New Zealand. ASP Conference Proceedings. Vol. 310. San Francisco: Astronomical Society of the Pacific. p. 403.
1341:
Usenko, I. A.; et al. (July 2011). "Spectroscopic studies of
Cepheids (S Cru, AP Pup, AX Cir, S TrA, T Cru, R Mus, S Mus, U Car) and semiregular bright supergiants (V382 Car, HD 75276, R Pup) in the southern hemisphere".
708:
of 0.19. A binary companion was first suspected in 1960, as the spectrum was considered to be composite and there is an ultraviolet excess. The companion was confirmed in 1982, and it was resolved using long baseline
1575:
Gallenne, A; Mérand, A; Kervella, P; Breitfelder, J; Le
Bouquin, J.-B; Monnier, J. D; Gieren, W; Pilecki, B; Pietrzyński, G (2013). "Multiplicity of Galactic Cepheids from long-baseline interferometry".
1438:
Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?",
931:
Klagyivik, P.; Szabados, L. (September 2009). "Observational studies of
Cepheid amplitudes. I. Period-amplitude relationships for Galactic Cepheids and interrelation of amplitudes".
1522:
Gallenne, A.; et al. (July 2015). "Robust high-contrast companion detection from interferometric observations. The CANDID algorithm and an application to six binary
Cepheids".
993:
Gallenne, A.; et al. (January 2014), "Multiplicity of
Galactic Cepheids from long-baseline interferometry. II. The Companion of AX Circini revealed with VLTI/PIONIER",
602:
2013:
1501:
1189:
Evans, Nancy Evans; Bond, Howard E; Schaefer, Gail H; Mason, Brian D; Karovska, Margarita; Tingle, Evan (2013). "Binary
Cepheids: Separations and Mass Ratios in 5 M
470:
1385:
Luck, R. E.; et al. (August 2011). "The
Distribution of the Elements in the Galactic Disk. II. Azimuthal and Radial Variation in Abundances from Cepheids".
1998:
1090:
Samus', N. N; Kazarovets, E. V; Durlevich, O. V; Kireeva, N. N; Pastukhova, E. N (2017). "General catalogue of variable stars: Version GCVS 5.1".
2008:
649:
1978:
1973:
1136:
de
Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",
1647:
2018:
1988:
31:
607:
1968:
664:
515:
814:
2003:
756:
674:. It has a nominal magnitude of 5.91, which is bright enough to be visible to the naked eye. Based upon an annual
1735:
1665:
801:
768:
598:
579:
1656:
855:
1993:
1786:
1640:
752:
590:
584:
96:
1768:
478:
317:
135:
1595:
1541:
1457:
1404:
1351:
1300:
1256:
1212:
1155:
1099:
1062:
1012:
950:
894:
833:
705:
697:
297:
229:
763:
of the system ranges from 5.69 to 6.19 over 5.273 days. The secondary companion, component B, is a
741:
594:
1611:
1585:
1557:
1531:
1473:
1447:
1420:
1394:
1367:
1318:
1290:
1228:
1202:
1171:
1145:
1115:
1028:
1002:
966:
940:
910:
884:
823:
764:
760:
250:
76:
1983:
1949:
1682:
1633:
724:
575:
342:
27:
1820:
1603:
1599:
1549:
1545:
1465:
1461:
1412:
1359:
1308:
1220:
1163:
1159:
1107:
1070:
1020:
1016:
958:
954:
902:
843:
838:
675:
637:
507:
445:
213:
1491:
629:
1929:
1710:
690:
458:
154:
52:
1251:
Petterson, O. K. L.; et al. (May 2004). Kurtz, Donald W.; Pollard, Karen R. (eds.).
1408:
1355:
1304:
1260:
1216:
1103:
1066:
898:
733:
710:
701:
681:
567:
362:
278:
221:
201:
189:
1962:
1725:
1705:
1700:
1690:
1424:
1416:
1371:
1313:
1278:
1224:
1119:
914:
667:
178:
130:
39:
1615:
1477:
1322:
1232:
1175:
1032:
970:
1869:
1810:
1715:
1695:
1561:
748:
548:
425:
398:
1607:
1553:
1469:
1167:
1024:
962:
848:
805:
1851:
1720:
660:
641:
500:
120:
109:
65:
1758:
1753:
1748:
1363:
1111:
1075:
1050:
906:
875:
Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation".
686:
555:
438:
405:
339:
236:
142:
1843:
1794:
1776:
1625:
1903:
1877:
671:
44:
1921:
1895:
1496:
859:
623:
492:
418:
241:
1536:
828:
1825:
1590:
1452:
1399:
1295:
1207:
1150:
1007:
945:
889:
636:
270:
1279:"Comparative statistics and origin of triple and quadruple stars"
1815:
1673:
689:
from the Earth. The system is moving closer with a heliocentric
645:
205:
193:
1629:
810:
Data
Release 2: Summary of the contents and survey properties"
1920:
1894:
1868:
1842:
1803:
1785:
1767:
1734:
1681:
1672:
804:; et al. (Gaia collaboration) (August 2018).
1283:Monthly Notices of the Royal Astronomical Society
1253:A spectroscopic study of southern binary Cepheids
1055:Monthly Notices of the Royal Astronomical Society
747:The primary, component A, is a yellow-white-hued
1272:
1270:
1044:
1042:
16:Binary star system in the constellation Circinus
1246:
1244:
1242:
1131:
1129:
926:
924:
988:
986:
984:
982:
980:
870:
868:
1641:
1502:Centre de données astronomiques de Strasbourg
1336:
1334:
1332:
70:−63° 48′ 35.4172″
8:
1917:
1891:
1865:
1839:
1678:
1648:
1634:
1626:
771:and an absolute magnitude of about −0.12.
1589:
1535:
1451:
1398:
1312:
1294:
1206:
1149:
1074:
1006:
944:
888:
847:
837:
827:
796:
794:
792:
790:
788:
786:
784:
30:J2000
2014:Objects with variable star designations
780:
185:
18:
650:Transiting Exoplanet Survey Satellite
7:
713:in 2014 and 2015. The system has an
1051:"The frequency of Cepheid binaries"
685:, it is located roughly 1,900
197:
14:
1945:
1944:
1314:10.1111/j.1365-2966.2008.13613.x
856:Gaia DR2 record for this source
220:1.7449 ± 0.3450
1999:Henry Draper Catalogue objects
1:
2009:Bright Star Catalogue objects
1578:Astronomy & Astrophysics
1524:Astronomy & Astrophysics
1440:Astronomy & Astrophysics
1138:Astronomy & Astrophysics
995:Astronomy & Astrophysics
815:Astronomy & Astrophysics
1979:Classical Cepheid variables
1608:10.1051/0004-6361/201322883
1554:10.1051/0004-6361/201525917
1470:10.1051/0004-6361/201118724
1168:10.1051/0004-6361/201219219
1025:10.1051/0004-6361/201322883
963:10.1051/0004-6361/200811464
849:10.1051/0004-6361/201833051
755:of F8 II, and it is a
2035:
1974:B-type main-sequence stars
1417:10.1088/0004-6256/142/2/51
1225:10.1088/0004-6256/146/4/93
933:Astronomy and Astrophysics
757:classical Cepheid variable
644:of AX Circini recorded by
1942:
1916:
1890:
1864:
1838:
1666:List of stars in Circinus
1663:
1657:Constellation of Circinus
1364:10.1134/S1063773711070061
1112:10.1134/S1063772917010085
907:10.1134/S1063773712050015
616:
573:
566:
541:
391:
386:
269:
265:
148:
141:
90:
24:
1387:The Astronomical Journal
1195:The Astronomical Journal
1600:2014A&A...561L...3G
1546:2015A&A...579A..68G
1462:2012A&A...542A.116A
1160:2012A&A...546A..61D
1076:10.1093/mnras/141.1.109
1049:Lloyd Evans, T (1968).
1017:2014A&A...561L...3G
955:2009A&A...504..959K
839:2018A&A...616A...1G
251:Absolute magnitude
77:Apparent magnitude
2019:Spectroscopic binaries
1989:Durchmusterung objects
1277:Tokovinin, A. (2008).
753:stellar classification
704:of 17.88 years and an
653:
640:
318:Longitude of the node
1969:F-type bright giants
698:spectroscopic binary
1409:2011AJ....142...51L
1356:2011AstL...37..499U
1305:2008MNRAS.389..925T
1261:2004ASPC..310..403P
1217:2013AJ....146...93E
1104:2017ARep...61...80S
1067:1968MNRAS.141..109L
899:2012AstL...38..331A
742:orbital inclination
617:Database references
516:Rotational velocity
235:approx. 1,900
21:
765:main-sequence star
761:apparent magnitude
693:of −21 km/s.
654:
568:Other designations
240:(approx. 600
200: −5.108
188: −4.779
131:Variable type
97:Spectral type
19:
2004:Hipparcos objects
1956:
1955:
1938:
1937:
1912:
1911:
1886:
1885:
1860:
1859:
1834:
1833:
1344:Astronomy Letters
1092:Astronomy Reports
877:Astronomy Letters
740:is the (unknown)
635:
634:
2026:
1948:
1947:
1918:
1892:
1866:
1840:
1679:
1650:
1643:
1636:
1627:
1620:
1619:
1593:
1572:
1566:
1565:
1539:
1519:
1513:
1512:
1510:
1508:
1488:
1482:
1481:
1455:
1435:
1429:
1428:
1402:
1382:
1376:
1375:
1338:
1327:
1326:
1316:
1298:
1274:
1265:
1264:
1248:
1237:
1236:
1210:
1186:
1180:
1179:
1153:
1133:
1124:
1123:
1087:
1081:
1080:
1078:
1046:
1037:
1036:
1010:
990:
975:
974:
948:
928:
919:
918:
892:
872:
863:
853:
851:
841:
831:
798:
767:with a class of
727:
684:
611:
593: 130701/2,
588:
536:
534:
490:
488:
381:
379:
356:
354:
347:
331:
329:
322:
310:
308:
291:
289:
199:
187:
171:
169:
103:
91:Characteristics
86:
80:
60:
55:
25:Observation data
22:
2034:
2033:
2029:
2028:
2027:
2025:
2024:
2023:
1959:
1958:
1957:
1952:
1934:
1930:Circinus Galaxy
1908:
1882:
1856:
1830:
1799:
1781:
1763:
1730:
1668:
1659:
1654:
1624:
1623:
1574:
1573:
1569:
1521:
1520:
1516:
1506:
1504:
1490:
1489:
1485:
1437:
1436:
1432:
1384:
1383:
1379:
1340:
1339:
1330:
1276:
1275:
1268:
1250:
1249:
1240:
1192:
1188:
1187:
1183:
1135:
1134:
1127:
1089:
1088:
1084:
1048:
1047:
1040:
992:
991:
978:
930:
929:
922:
874:
873:
866:
802:Brown, A. G. A.
800:
799:
782:
777:
759:. The combined
722:
691:radial velocity
679:
612:
606:
583:
561:
558:
532:
530:
522: sin
486:
484:
459:Surface gravity
451:
448:
431:
428:
411:
408:
377:
375:
371:
369:
352:
350:
337:
327:
325:
315:
306:
304:
287:
285:
256:
239:
196:
167:
165:
160:
155:Radial velocity
101:
84:
75:
58:
53:Right ascension
51:
26:
17:
12:
11:
5:
2032:
2030:
2022:
2021:
2016:
2011:
2006:
2001:
1996:
1991:
1986:
1981:
1976:
1971:
1961:
1960:
1954:
1953:
1943:
1940:
1939:
1936:
1935:
1933:
1932:
1926:
1924:
1914:
1913:
1910:
1909:
1907:
1906:
1900:
1898:
1888:
1887:
1884:
1883:
1881:
1880:
1874:
1872:
1862:
1861:
1858:
1857:
1855:
1854:
1848:
1846:
1836:
1835:
1832:
1831:
1829:
1828:
1823:
1818:
1813:
1807:
1805:
1801:
1800:
1798:
1797:
1791:
1789:
1783:
1782:
1780:
1779:
1773:
1771:
1765:
1764:
1762:
1761:
1756:
1751:
1746:
1740:
1738:
1732:
1731:
1729:
1728:
1723:
1718:
1713:
1708:
1703:
1698:
1693:
1687:
1685:
1676:
1670:
1669:
1664:
1661:
1660:
1655:
1653:
1652:
1645:
1638:
1630:
1622:
1621:
1567:
1514:
1483:
1430:
1377:
1350:(7): 499–507.
1328:
1289:(2): 925–938.
1266:
1238:
1190:
1181:
1125:
1082:
1038:
976:
939:(3): 959–972.
920:
864:
779:
778:
776:
773:
734:semimajor axis
711:interferometry
702:orbital period
676:parallax shift
663:system in the
633:
632:
627:
619:
618:
614:
613:
605: 252928,
574:
571:
570:
564:
563:
559:
556:
552:
544:
543:
539:
538:
528:
511:
510:
504:
496:
495:
482:
474:
473:
467:
454:
453:
449:
446:
442:
434:
433:
429:
426:
422:
414:
413:
409:
406:
402:
394:
393:
389:
388:
384:
383:
373:
367:
363:Semi-amplitude
358:
357:
348:
334:
333:
323:
312:
311:
302:
293:
292:
283:
274:
273:
267:
266:
263:
262:
259:
254:
246:
245:
233:
225:
224:
218:
209:
208:
183:
174:
173:
163:
158:
150:
149:
146:
145:
139:
138:
133:
127:
126:
123:
116:
115:
112:
105:
104:
99:
93:
92:
88:
87:
81:
72:
71:
68:
62:
61:
59:14 52 35.25324
56:
48:
47:
42:
36:
35:
15:
13:
10:
9:
6:
4:
3:
2:
2031:
2020:
2017:
2015:
2012:
2010:
2007:
2005:
2002:
2000:
1997:
1995:
1994:Gould objects
1992:
1990:
1987:
1985:
1982:
1980:
1977:
1975:
1972:
1970:
1967:
1966:
1964:
1951:
1941:
1931:
1928:
1927:
1925:
1923:
1919:
1915:
1905:
1902:
1901:
1899:
1897:
1893:
1889:
1879:
1876:
1875:
1873:
1871:
1870:Star clusters
1867:
1863:
1853:
1850:
1849:
1847:
1845:
1841:
1837:
1827:
1824:
1822:
1819:
1817:
1814:
1812:
1809:
1808:
1806:
1802:
1796:
1793:
1792:
1790:
1788:
1784:
1778:
1775:
1774:
1772:
1770:
1766:
1760:
1757:
1755:
1752:
1750:
1747:
1745:
1742:
1741:
1739:
1737:
1733:
1727:
1724:
1722:
1719:
1717:
1714:
1712:
1709:
1707:
1704:
1702:
1699:
1697:
1694:
1692:
1689:
1688:
1686:
1684:
1680:
1677:
1675:
1671:
1667:
1662:
1658:
1651:
1646:
1644:
1639:
1637:
1632:
1631:
1628:
1617:
1613:
1609:
1605:
1601:
1597:
1592:
1587:
1583:
1579:
1571:
1568:
1563:
1559:
1555:
1551:
1547:
1543:
1538:
1533:
1529:
1525:
1518:
1515:
1503:
1499:
1498:
1493:
1487:
1484:
1479:
1475:
1471:
1467:
1463:
1459:
1454:
1449:
1445:
1441:
1434:
1431:
1426:
1422:
1418:
1414:
1410:
1406:
1401:
1396:
1392:
1388:
1381:
1378:
1373:
1369:
1365:
1361:
1357:
1353:
1349:
1345:
1337:
1335:
1333:
1329:
1324:
1320:
1315:
1310:
1306:
1302:
1297:
1292:
1288:
1284:
1280:
1273:
1271:
1267:
1262:
1258:
1254:
1247:
1245:
1243:
1239:
1234:
1230:
1226:
1222:
1218:
1214:
1209:
1204:
1200:
1196:
1185:
1182:
1177:
1173:
1169:
1165:
1161:
1157:
1152:
1147:
1143:
1139:
1132:
1130:
1126:
1121:
1117:
1113:
1109:
1105:
1101:
1097:
1093:
1086:
1083:
1077:
1072:
1068:
1064:
1060:
1056:
1052:
1045:
1043:
1039:
1034:
1030:
1026:
1022:
1018:
1014:
1009:
1004:
1000:
996:
989:
987:
985:
983:
981:
977:
972:
968:
964:
960:
956:
952:
947:
942:
938:
934:
927:
925:
921:
916:
912:
908:
904:
900:
896:
891:
886:
882:
878:
871:
869:
865:
861:
857:
850:
845:
840:
835:
830:
825:
821:
817:
816:
811:
809:
803:
797:
795:
793:
791:
789:
787:
785:
781:
774:
772:
770:
766:
762:
758:
754:
750:
745:
743:
739:
735:
731:
726:
720:
716:
712:
707:
703:
699:
694:
692:
688:
683:
677:
673:
669:
668:constellation
666:
662:
658:
651:
647:
643:
639:
631:
628:
626:
625:
621:
620:
615:
610:J14526-6349AB
609:
604:
600:
597: 72773,
596:
592:
586:
581:
577:
572:
569:
565:
562:
553:
551:
550:
546:
545:
540:
529:
527:
525:
521:
517:
513:
512:
509:
505:
503:
502:
498:
497:
494:
483:
481:
480:
476:
475:
472:
468:
466:
464:
460:
456:
455:
452:
443:
441:
440:
436:
435:
432:
423:
421:
420:
416:
415:
412:
403:
401:
400:
396:
395:
390:
385:
374:
365:
364:
360:
359:
349:
346:
344:
341:
336:
335:
324:
321:
319:
314:
313:
303:
301:
299:
295:
294:
284:
282:
280:
276:
275:
272:
268:
264:
260:
258:
252:
248:
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1821:PSR B1509−58
1811:Circinus X-1
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749:bright giant
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706:eccentricity
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601: 5527,
547:
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298:Eccentricity
296:
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212:
177:
153:
102:F8 II + B6 V
1852:HD 129445 b
1193:Binaries".
1061:: 109–142.
687:light-years
661:binary star
642:Light curve
506:−0.05
501:Metallicity
479:Temperature
444:2,050
424:45.68
404:11.56
121:color index
110:color index
85:(5.69–6.19)
66:Declination
20:AX Circini
1963:Categories
1844:Exoplanets
1537:1505.02715
883:(5): 331.
829:1804.09365
775:References
723:6.05
696:This is a
657:AX Circini
554:5.57
537: km/s
469:2.00
461:(log
439:Luminosity
355:60 JD
340:Periastron
172: km/s
143:Astrometry
1591:1312.1950
1507:28 August
1453:1204.2459
1425:119288363
1400:1106.0182
1393:(2): 12.
1372:122968535
1296:0806.3263
1208:1307.7123
1201:(4): 93.
1151:1208.3048
1120:125853869
1098:(1): 80.
1008:1312.1950
946:0908.3561
915:119257644
890:1108.4971
769:B6 V
721:value of
680:1.7
587:−63° 1029
576:26 G. Cir
372:(primary)
351:2,448,500
290:25 d
79: (V)
1984:Circinus
1950:Category
1922:Galaxies
1904:NGC 5315
1878:NGC 5823
1736:Variable
1616:14282671
1492:"26 Cir"
1478:53666672
1446:: A116,
1323:16452670
1233:34133110
1176:59451347
1033:14282671
971:18283579
728:, where
700:with an
672:Circinus
665:southern
560:☉
542:AX Cir B
450:☉
430:☉
410:☉
392:AX Cir A
253: (M
230:Distance
214:Parallax
45:Circinus
1896:Nebulae
1596:Bibcode
1562:1118066
1542:Bibcode
1458:Bibcode
1405:Bibcode
1352:Bibcode
1301:Bibcode
1257:Bibcode
1213:Bibcode
1156:Bibcode
1100:Bibcode
1063:Bibcode
1013:Bibcode
951:Bibcode
895:Bibcode
834:Bibcode
751:with a
732:is the
387:Details
32:Equinox
1795:129445
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1497:SIMBAD
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652:(TESS)
624:SIMBAD
580:AX Cir
491:
419:Radius
332:°
279:Period
34:J2000
1826:WR 66
1804:Other
1683:Bayer
1674:Stars
1612:S2CID
1586:arXiv
1558:S2CID
1532:arXiv
1474:S2CID
1448:arXiv
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1421:S2CID
1395:arXiv
1368:S2CID
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1291:arXiv
1229:S2CID
1203:arXiv
1172:S2CID
1146:arXiv
1116:S2CID
1029:S2CID
1003:arXiv
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967:S2CID
941:arXiv
911:S2CID
885:arXiv
854:
824:arXiv
659:is a
485:5,443
343:epoch
286:6,532
271:Orbit
261:−3.37
198:Dec.:
166:−20.9
136:δ Cep
125:+0.8
114:+0.2
83:5.91
28:Epoch
1816:MN18
1777:5632
1509:2018
1035:, L3
808:Gaia
736:and
717:sin
646:NASA
630:data
549:Mass
399:Mass
382:km/s
376:10.0
309:0.02
305:0.19
119:B−V
108:U−B
1604:doi
1582:561
1550:doi
1528:579
1466:doi
1444:542
1413:doi
1391:142
1360:doi
1309:doi
1287:389
1221:doi
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1071:doi
1059:141
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937:504
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858:at
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682:mas
678:of
670:of
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603:SAO
595:HIP
535:0.4
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508:dex
471:cgs
380:0.5
345:(T)
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320:(Ω)
300:(e)
281:(P)
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216:(π)
202:mas
190:mas
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