32:
1955:
39:
748:
which indicated a companion star was present were not definitive. With an orbit and a parallax the sum of the masses of the two stars can be determined via a
693:
around 0.35. The secondary is about 3.3 magnitudes dimmer than the primary and estimated as type B9 based on the flux of far-ultraviolet radiation.
1556:
1121:
610:
504:
1224:
1135:
Soubiran, Caroline; Le
Campion, Jean-François; Brouillet, Nathalie; Chemin, Laurent (2016). "The PASTEL catalogue: 2016 version".
2002:
2012:
1459:
727:
744:
using observations from the Navy
Precision Optical Interferometer. This detection was significant as observations with the
1549:
1334:
Hutter, D. J.; Zavala, R. T.; Tycner, C.; Benson, J. A.; Hummel, C. A.; Sanborn, J.; Franz, O. G.; Johnston, K. J. (2016).
1295:"Ultraviolet and Optical Studies of Binaries with Luminous Cool Primaries and Hot Companions. V. The Entire IUE Sample"
1336:"Surveying the Bright Stars by Optical Interferometry. I. A Search for Multiplicity among Stars of Spectral Types F-K"
928:
Ducati, J. R. (2002). "VizieR Online Data
Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".
1997:
1987:
1982:
1958:
1542:
60:
1072:
Baines, Ellyn K.; Clark, James H., III; Schmitt, Henrique R.; Stone, Jordan M.; von Braun, Kaspar (2023-12-01).
1002:
844:
890:
Keenan, Philip C.; McNeil, Raymond C. (1989). "The
Perkins catalog of revised MK types for the cooler stars".
1977:
549:
1717:
1581:
1188:
De
Medeiros, J. R.; Mayor, M. (1999). "A catalog of rotational and radial velocities for evolved stars".
586:
2007:
700:
of +4.22 and is radiating about 1,315 times the luminosity of the Sun from its outer atmosphere at an
1648:
697:
602:
1481:
741:
740:
The secondary was directly detected with a magnitude difference of 3.6 at a separation of about 17
1576:
1992:
1565:
745:
712:
654:
631:
606:
590:
410:
134:
73:
1074:"33 New Stellar Angular Diameters from the NPOI, and Nearly 180 NPOI Diameters as an Ensemble"
1843:
1115:
701:
643:
512:
377:
1263:
1211:
1158:
874:
820:
2017:
1504:
1439:
1406:
1357:
1306:
1259:
1207:
1154:
1085:
1027:
977:
937:
899:
870:
816:
690:
682:
350:
253:
1240:; Torres, G.; Udry, S. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits".
1236:
Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; Levato, H.;
8:
1777:
598:
1508:
1443:
1410:
1361:
1310:
1089:
1031:
981:
941:
903:
1757:
1732:
1520:
1469:
1375:
1347:
1275:
1249:
1197:
1170:
1144:
1045:
993:
967:
834:
806:
749:
594:
274:
105:
1912:
1600:
1524:
1455:
1379:
1279:
1174:
1103:
1049:
1040:
1015:
997:
838:
395:
122:
56:
1370:
1335:
1727:
1722:
1512:
1447:
1414:
1365:
1314:
1267:
1215:
1162:
1093:
1035:
985:
907:
824:
716:
658:
541:
479:
237:
1166:
829:
790:
1772:
1271:
492:
336:
178:
81:
752:. This eventually can yield a precise mass for the evolved giant primary star.
1712:
1516:
1098:
1073:
723:
686:
662:
582:
573:
322:
245:
225:
213:
1451:
989:
958:
Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation".
1971:
1628:
1237:
1107:
651:
202:
68:
1907:
1832:
1808:
1803:
708:
452:
31:
1534:
1219:
1882:
1623:
1618:
1608:
1254:
1202:
1016:"Hipparcos Photocentric Orbits of 72 Single-lined Spectroscopic Binaries"
705:
647:
534:
363:
156:
145:
94:
1892:
1877:
1872:
1697:
1671:
1633:
666:
465:
392:
260:
166:
127:
38:
1818:
1813:
1795:
1767:
1762:
1752:
1638:
1887:
1856:
1851:
1707:
1702:
1666:
1419:
1394:
1352:
1319:
1294:
1149:
911:
811:
972:
1938:
1681:
1661:
1656:
1395:"The Fine Guidance Sensor Orbit of the G4 Bright Giant HD 173764"
1134:
861:
Mallik, Sushma V. (December 1999), "Lithium abundance and mass",
1930:
1747:
1742:
1737:
1676:
848:
625:
526:
435:
265:
788:
1902:
1897:
795:
Data
Release 3. Summary of the content and survey properties"
294:
1235:
730:, which gives it a physical radius of approximately 49
1591:
229:
217:
670:
665:
as seen from Earth, it is located approximately 670
1393:
Parsons, S. B.; Franz, O. G.; Wassermann, L. H. (2005).
1333:
789:
Vallenari, A.; et al. (Gaia collaboration) (2023).
1495:
Wagman, M. (August 1987). "Flamsteed's
Missing Stars".
1071:
1392:
1969:
1187:
957:
1550:
1181:
1190:Astronomy and Astrophysics Supplement Series
1120:: CS1 maint: multiple names: authors list (
923:
921:
889:
885:
883:
704:of 4,951 K. This yellow-hued star is a
99:−04° 44′ 52.342″
1564:
1299:The Astrophysical Journal Supplement Series
1293:Parsons, Sidney B.; Ake, Thomas B. (1998).
1286:
1128:
1013:
930:CDS/ADC Collection of Electronic Catalogues
892:The Astrophysical Journal Supplement Series
1557:
1543:
1292:
1794:
1418:
1369:
1351:
1318:
1253:
1201:
1148:
1097:
1039:
971:
918:
880:
854:
828:
810:
59:J2000
1386:
1340:Astrophysical Journal Supplement Series
1229:
755:Beta Scuti was a latter designation of
209:
1970:
1929:
1494:
1433:
1327:
1067:
1065:
1063:
1061:
1059:
953:
951:
927:
860:
1538:
784:
782:
780:
778:
776:
774:
772:
728:Navy Precision Optical Interferometer
1497:Journal for the History of Astronomy
1056:
948:
613: 142618, CCDM 18472-0445
221:
13:
769:
676:
14:
2029:
1954:
1953:
37:
30:
16:Star in the constellation Scutum
1488:
1427:
845:Gaia DR3 record for this source
244:4.8549 ± 0.3403
2003:Henry Draper Catalogue objects
1007:
1:
2013:Bright Star Catalogue objects
762:
696:The primary component has an
48:Location of β Scuti (circled)
1137:Astronomy & Astrophysics
7:
1582:Scutum in Chinese astronomy
1167:10.1051/0004-6361/201628497
830:10.1051/0004-6361/202243940
737:at the estimated distance.
10:
2034:
1517:10.1177/002182868701800305
1272:10.1051/0004-6361:20041213
1242:Astronomy and Astrophysics
1041:10.1088/0004-6256/145/3/81
863:Astronomy and Astrophysics
799:Astronomy and Astrophysics
1951:
1925:
1865:
1842:
1831:
1790:
1690:
1647:
1599:
1590:
1572:
1452:10.1007/978-94-009-9836-0
1434:Heintz, Wulff D. (1978).
1371:10.3847/0067-0049/227/1/4
990:10.1134/S1063773712050015
698:apparent visual magnitude
618:
579:
572:
568:
429:
424:
293:
289:
172:
165:
116:
53:
24:
1099:10.3847/1538-3881/ad08be
1078:The Astronomical Journal
1020:The Astronomical Journal
1718:2MASS J18450079–1409036
1577:List of stars in Scutum
1566:Constellation of Scutum
1436:Double Stars - Springer
1264:2004A&A...424..727P
1212:1999A&AS..139..433D
1159:2016A&A...591A.118S
875:1999A&A...352..495M
821:2023A&A...674A...1G
657:. Based upon an annual
650:system in the southern
275:Absolute magnitude
123:Evolutionary stage
106:Apparent magnitude
1998:Durchmusterung objects
1988:Scutum (constellation)
1983:Spectroscopic binaries
746:Hubble Space Telescope
713:stellar classification
411:Argument of periastron
719:was measured at 2.121
702:effective temperature
378:Longitude of the node
1978:G-type bright giants
1399:Astronomical Journal
1225:Vizier catalog entry
1014:Ren, Shulin (2013).
1003:Vizier catalog entry
715:of G4 IIa. Its
683:spectroscopic binary
1778:Stephenson 2 DFK 49
1509:1987JHA....18..209W
1444:1978GAM....15.....H
1411:2005AJ....129.1700P
1362:2016ApJS..227....4H
1311:1998ApJS..119...83P
1220:10.1051/aas:1999401
1090:2023AJ....166..268B
1032:2013AJ....145...81R
982:2012AstL...38..331A
942:2002yCat.2237....0D
904:1989ApJS...71..245K
646:from β Scuti, is a
619:Database references
597: 05122-01426,
550:Rotational velocity
224: −16.398
21:
1758:Stephenson 2 DFK 1
750:dynamical parallax
574:Other designations
212: −7.972
135:Spectral type
19:
2008:Hipparcos objects
1965:
1964:
1947:
1946:
1921:
1920:
1913:Wild Duck Cluster
1827:
1826:
1786:
1785:
1461:978-90-277-0886-1
960:Astronomy Letters
689:of 2.3 years and
637:
636:
2025:
1957:
1956:
1927:
1926:
1840:
1839:
1792:
1791:
1597:
1596:
1559:
1552:
1545:
1536:
1535:
1529:
1528:
1492:
1486:
1485:
1479:
1475:
1473:
1465:
1438:. Vol. 15.
1431:
1425:
1424:
1422:
1390:
1384:
1383:
1373:
1355:
1331:
1325:
1324:
1322:
1290:
1284:
1283:
1257:
1255:astro-ph/0406573
1233:
1227:
1223:
1205:
1203:astro-ph/0608248
1185:
1179:
1178:
1152:
1132:
1126:
1125:
1119:
1111:
1101:
1069:
1054:
1053:
1043:
1011:
1005:
1001:
975:
955:
946:
945:
925:
916:
915:
887:
878:
877:
858:
852:
842:
832:
814:
786:
742:milli-arcseconds
722:
717:angular diameter
524:
522:
477:
475:
450:
449:
448:
415:
400:
382:
341:
223:
211:
195:
193:
117:Characteristics
109:
89:
84:
54:Observation data
41:
34:
22:
18:
2033:
2032:
2028:
2027:
2026:
2024:
2023:
2022:
1968:
1967:
1966:
1961:
1943:
1917:
1861:
1834:
1823:
1782:
1773:IRAS 18357-0604
1686:
1643:
1586:
1568:
1563:
1533:
1532:
1493:
1489:
1477:
1476:
1467:
1466:
1462:
1432:
1428:
1391:
1387:
1332:
1328:
1291:
1287:
1234:
1230:
1186:
1182:
1133:
1129:
1113:
1112:
1070:
1057:
1012:
1008:
956:
949:
926:
919:
888:
881:
859:
855:
787:
770:
765:
736:
733:
724:milliarcseconds
720:
679:
677:Characteristics
614:
556: sin
520:
518:
493:Surface gravity
485:
482:
473:
471:
458:
455:
446:
444:
443:
441:
416:
408:
390:
375:
337:Semi-major axis
334:
280:
264:(210 ± 10
263:
220:
191:
189:
184:
179:Radial velocity
104:
87:
82:Right ascension
80:
55:
49:
47:
46:
45:
44:
43:
42:
17:
12:
11:
5:
2031:
2021:
2020:
2015:
2010:
2005:
2000:
1995:
1990:
1985:
1980:
1963:
1962:
1952:
1949:
1948:
1945:
1944:
1942:
1941:
1935:
1933:
1923:
1922:
1919:
1918:
1916:
1915:
1910:
1905:
1900:
1895:
1890:
1885:
1880:
1875:
1869:
1867:
1863:
1862:
1860:
1859:
1854:
1848:
1846:
1837:
1829:
1828:
1825:
1824:
1822:
1821:
1816:
1811:
1806:
1800:
1798:
1788:
1787:
1784:
1783:
1781:
1780:
1775:
1770:
1765:
1760:
1755:
1750:
1745:
1740:
1735:
1733:PSR J1841−0500
1730:
1725:
1720:
1715:
1710:
1705:
1700:
1694:
1692:
1688:
1687:
1685:
1684:
1679:
1674:
1669:
1664:
1659:
1653:
1651:
1645:
1644:
1642:
1641:
1636:
1631:
1626:
1621:
1616:
1611:
1605:
1603:
1594:
1588:
1587:
1585:
1584:
1579:
1573:
1570:
1569:
1562:
1561:
1554:
1547:
1539:
1531:
1530:
1487:
1478:|journal=
1460:
1426:
1420:10.1086/427853
1385:
1326:
1320:10.1086/313152
1285:
1248:(2): 727–732.
1238:Morrell, N. I.
1228:
1180:
1127:
1055:
1006:
947:
917:
912:10.1086/191373
879:
853:
767:
766:
764:
761:
734:
731:
687:orbital period
678:
675:
659:parallax shift
635:
634:
629:
621:
620:
616:
615:
609: 173764,
580:
577:
576:
570:
569:
566:
565:
562:
545:
544:
538:
530:
529:
516:
508:
507:
501:
488:
487:
483:
480:
469:
461:
460:
456:
453:
439:
431:
430:
427:
426:
422:
421:
418:
405:
404:
401:
387:
386:
383:
372:
371:
368:
359:
358:
355:
346:
345:
342:
331:
330:
327:
318:
317:
314:
308:
307:
304:
298:
297:
291:
290:
287:
286:
283:
278:
270:
269:
259:670 ± 50
257:
249:
248:
242:
233:
232:
207:
198:
197:
187:
182:
174:
173:
170:
169:
163:
162:
159:
152:
151:
148:
141:
140:
137:
131:
130:
125:
119:
118:
114:
113:
110:
101:
100:
97:
91:
90:
85:
77:
76:
71:
65:
64:
51:
50:
36:
35:
29:
28:
27:
26:
25:
15:
9:
6:
4:
3:
2:
2030:
2019:
2016:
2014:
2011:
2009:
2006:
2004:
2001:
1999:
1996:
1994:
1993:Bayer objects
1991:
1989:
1986:
1984:
1981:
1979:
1976:
1975:
1973:
1960:
1950:
1940:
1937:
1936:
1934:
1932:
1928:
1924:
1914:
1911:
1909:
1906:
1904:
1901:
1899:
1896:
1894:
1891:
1889:
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1884:
1881:
1879:
1876:
1874:
1871:
1870:
1868:
1864:
1858:
1855:
1853:
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1849:
1847:
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1841:
1838:
1836:
1830:
1820:
1817:
1815:
1812:
1810:
1807:
1805:
1802:
1801:
1799:
1797:
1793:
1789:
1779:
1776:
1774:
1771:
1769:
1766:
1764:
1761:
1759:
1756:
1754:
1751:
1749:
1746:
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1741:
1739:
1736:
1734:
1731:
1729:
1726:
1724:
1721:
1719:
1716:
1714:
1711:
1709:
1706:
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1701:
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1670:
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1610:
1607:
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1602:
1598:
1595:
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1578:
1575:
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1560:
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1502:
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1471:
1463:
1457:
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1437:
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1421:
1416:
1412:
1408:
1404:
1400:
1396:
1389:
1381:
1377:
1372:
1367:
1363:
1359:
1354:
1349:
1345:
1341:
1337:
1330:
1321:
1316:
1312:
1308:
1304:
1300:
1296:
1289:
1281:
1277:
1273:
1269:
1265:
1261:
1256:
1251:
1247:
1243:
1239:
1232:
1226:
1221:
1217:
1213:
1209:
1204:
1199:
1195:
1191:
1184:
1176:
1172:
1168:
1164:
1160:
1156:
1151:
1146:
1142:
1138:
1131:
1123:
1117:
1109:
1105:
1100:
1095:
1091:
1087:
1083:
1079:
1075:
1068:
1066:
1064:
1062:
1060:
1051:
1047:
1042:
1037:
1033:
1029:
1025:
1021:
1017:
1010:
1004:
999:
995:
991:
987:
983:
979:
974:
969:
965:
961:
954:
952:
943:
939:
935:
931:
924:
922:
913:
909:
905:
901:
897:
893:
886:
884:
876:
872:
868:
864:
857:
850:
846:
840:
836:
831:
826:
822:
818:
813:
808:
804:
800:
796:
794:
785:
783:
781:
779:
777:
775:
773:
768:
760:
758:
753:
751:
747:
743:
738:
729:
725:
718:
714:
710:
707:
703:
699:
694:
692:
688:
684:
674:
672:
668:
664:
661:of 4.85
660:
656:
653:
652:constellation
649:
645:
641:
633:
630:
628:
627:
623:
622:
617:
612:
608:
604:
601: 92175,
600:
596:
593: 25730,
592:
588:
584:
578:
575:
571:
567:
564:7.8 km/s
563:
561:
559:
555:
551:
547:
546:
543:
539:
537:
536:
532:
531:
528:
517:
515:
514:
510:
509:
506:
502:
500:
498:
494:
490:
489:
486:
470:
468:
467:
463:
462:
459:
440:
438:
437:
433:
432:
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419:
414:
412:
407:
406:
402:
399:
397:
394:
389:
388:
384:
381:
379:
374:
373:
369:
367:
365:
361:
360:
356:
354:
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1908:Stephenson 2
1804:BD-11 4672 b
1728:PSR B1829−10
1723:PSR B1828−11
1613:
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709:bright giant
695:
691:eccentricity
680:
639:
638:
624:
605: 7063,
589: 1489,
557:
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533:
511:
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491:
464:
434:
409:
391:
376:
362:
351:Eccentricity
349:
335:
321:
316:Beta Scuti B
311:
306:Beta Scuti A
301:
273:
252:
236:
201:
177:
88:18 47 10.474
2018:TIC objects
1883:Alicante 10
1405:(3): 1700.
869:: 495–507,
667:light years
648:binary star
540:-0.16
535:Metallicity
513:Temperature
417:(secondary)
385:288.1°
370:105.9°
364:Inclination
157:color index
146:color index
95:Declination
1972:Categories
1893:Messier 26
1878:Alicante 8
1873:Alicante 7
1796:Exoplanets
1713:IRC −10414
1698:BD-11 4672
1503:(3): 212.
1353:1609.05254
1196:(3): 433.
1150:1605.07384
1084:(6): 268.
966:(5): 331.
812:2208.00211
763:References
681:This is a
640:Beta Scuti
585:-04°4582,
503:0.94
495:(log
466:Luminosity
420:33.9°
393:Periastron
196: km/s
167:Astrometry
128:Giant star
1819:CoRoT-17b
1814:CoRoT-16b
1768:RSGC1-F02
1763:RSGC1-F01
1753:WR 121-16
1525:118445625
1480:ignored (
1470:cite book
1380:118803592
1305:(1): 83.
1280:119387088
1175:119258214
1108:0004-6256
1050:120199240
1026:(3): 81.
998:119257644
973:1108.4971
839:244398875
757:6 Aquilae
669:from the
644:Latinized
403:2422480.9
312:Companion
108: (V)
1959:Category
1888:Mercer 3
1835:clusters
1708:CoRoT-17
1703:CoRoT-16
1649:Variable
1346:(1): 4.
1143:: A118.
735:☉
685:with an
484:☉
457:☉
329:834 days
277: (M
254:Distance
238:Parallax
20:β Scuti
1939:IC 1295
1931:Nebulae
1505:Bibcode
1440:Bibcode
1407:Bibcode
1358:Bibcode
1307:Bibcode
1260:Bibcode
1208:Bibcode
1155:Bibcode
1086:Bibcode
1028:Bibcode
978:Bibcode
938:Bibcode
900:Bibcode
898:: 245.
871:Bibcode
817:Bibcode
726:by the
711:with a
581:β Sct,
425:Details
344:2.8 mas
302:Primary
61:Equinox
1748:WR 120
1743:WR 119
1738:WR 114
1523:
1458:
1378:
1278:
1173:
1106:
1048:
996:
849:VizieR
837:
805:: A1.
721:
706:G-type
655:Scutum
626:SIMBAD
525:
478:
451:
436:Radius
323:Period
190:−28.75
161:+1.09
150:+0.84
139:G4IIa
74:Scutum
63:J2000
1903:RSGC3
1898:RSGC1
1866:Other
1691:Other
1601:Bayer
1592:Stars
1521:S2CID
1376:S2CID
1348:arXiv
1276:S2CID
1250:arXiv
1198:arXiv
1171:S2CID
1145:arXiv
1046:S2CID
994:S2CID
968:arXiv
843:
835:S2CID
807:arXiv
519:4,951
472:1,315
447:−3.72
445:+3.24
442:49.26
396:epoch
357:0.350
295:Orbit
285:−2.99
222:Dec.:
112:4.22
57:Epoch
1857:6712
1852:6649
1833:Star
1682:V479
1677:V452
1672:V373
1482:help
1456:ISBN
1122:link
1104:ISSN
934:2237
793:Gaia
632:data
194:4.88
155:B−V
144:U−B
1844:NGC
1513:doi
1448:doi
1415:doi
1403:129
1366:doi
1344:227
1315:doi
1303:119
1268:doi
1246:424
1216:doi
1194:139
1163:doi
1141:591
1094:doi
1082:166
1036:doi
1024:145
986:doi
908:doi
867:352
847:at
825:doi
803:674
671:Sun
663:mas
611:SAO
599:HIP
595:GSC
587:FK5
542:dex
505:cgs
476:186
413:(ω)
398:(T)
380:(Ω)
366:(i)
353:(e)
339:(a)
325:(P)
246:mas
240:(π)
226:mas
214:mas
210:RA:
205:(μ)
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1667:UY
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266:pc
261:ly
230:yr
218:yr
181:(R
1809:c
1662:S
1657:R
1639:η
1634:ζ
1629:ε
1624:δ
1619:γ
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1609:α
1558:e
1551:t
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279:V
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216:/
192:±
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183:v
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