32:
3576:
910:
39:
778:
1230:
Mourard, D.; Monnier, J. D.; Meilland, A.; Gies, D.; Millour, F.; Benisty, M.; Che, X.; Grundstrom, E. D.; Ligi, R.; Schaefer, G.; Baron, F.; Kraus, S.; Zhao, M.; Pedretti, E.; Berio, P.; Clausse, J. M.; Nardetto, N.; Perraut, K.; Spang, A.; Stee, P.; Tallon-Bosc, I.; McAlister, H.; Ten
Brummelaar,
932:
with both rapid and longterm variations in its brightness and spectrum. Variations occur on a daily timescale which may be related to the rotation of the primary star. Any variations originating with the secondary are difficult to detect due to its comparative faintness. Slower variations,
933:
including deep fades, are also seen. Some of the variations may correspond to the orbital period, possibly eclipses of gas streams or hot spots, but the occasional deep fades do not match any particular orbital phase. The variations are classified as
1478:
Zorec, J.; Frémat, Y.; Domiciano De Souza, A.; Royer, F.; Cidale, L.; Hubert, A.-M.; Semaan, T.; Martayan, C.; Cochetti, Y. R.; Arias, M. L.; Aidelman, Y.; Stee, P. (2017). "Critical study of the distribution of rotational velocities of Be stars".
862:. The binary orbit, the spin of the primary star, and the disk are all seen nearly edge-on. There are no eclipses, but models of the system show that the disk significantly obscures the primary star. The primary formed as a 3.8
1422:
Schootemeijer, A.; Götberg, Y.; De Mink, S. E.; Gies, D.; Zapartas, E. (2018). "Clues about the scarcity of stripped-envelope stars from the evolutionary state of the sdO+Be binary system φ Persei".
1585:
Božić, H.; Harmanec, P.; Horn, J.; Koubský, P.; Scholz, G.; McDavid, D.; Hubert, A. M.; Hubert, H. (December 1995). "Toward a consistent model of the B0.5IVe + sdO binary φ Persei".
897:, which suggests it may have evolved to helium shell burning. Although the subdwarf has a bolometric luminosity about half that of the primary, it emits most of its radiation as
1691:
614:
495:
702:
3638:
1330:
Gies, Douglas R.; Bagnuolo, William G.; Ferrara, Elizabeth C.; Kaye, Anthony B.; Thaller, Michelle L.; Penny, Laura R.; Peters, Geraldine J. (1998).
3628:
3623:
1379:
1684:
1169:
Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data
Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)".
3613:
3608:
3579:
1677:
1295:
3633:
60:
1196:
Hoffleit, D.; Warren, W. H. (1995). "VizieR Online Data
Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)".
518:
3546:
1716:
988:
678:
3618:
3603:
934:
811:
162:
1139:
Ducati, J. R. (2002). "VizieR Online Data
Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".
3648:
2068:
957:
694:
1711:
1700:
758:
73:
3598:
3246:
2893:
1332:"Hubble Space Telescope Goddard High Resolution Spectrograph Observations of the Be + sdO Binary φ Persei"
747:
686:
682:
125:
3643:
3128:
2490:
1863:
961:
876:, hotter than the primary but smaller and less massive. It is proposed that it is the core of a 7
851:
840:
670:
622:
503:
345:
3057:
3052:
3047:
3207:
3022:
1613:
1548:
1498:
1441:
1343:
1299:
1254:
1205:
1178:
1148:
1097:
815:
786:
249:
1383:
690:
3067:
3103:
3042:
2470:
2460:
2455:
2450:
2445:
2440:
2435:
2416:
2411:
2406:
2396:
2386:
2381:
2376:
2371:
2366:
2361:
2356:
2351:
2336:
2326:
2321:
2316:
2311:
2306:
1629:
1564:
1538:
1488:
1457:
1431:
1361:
1272:
1244:
1113:
1087:
1033:
1009:
914:
859:
698:
270:
105:
2987:
2301:
2296:
2291:
2281:
2276:
2271:
2266:
2261:
2256:
2251:
2246:
2236:
2226:
2221:
2216:
2211:
2206:
2201:
2196:
2191:
2186:
2181:
2176:
2166:
2161:
2156:
2151:
2146:
2141:
2136:
2131:
2116:
723:
3261:
2966:
2961:
2951:
2941:
2936:
2931:
2916:
2911:
2906:
2901:
2883:
2878:
2873:
2868:
2863:
2858:
2853:
2848:
2843:
2838:
2833:
2828:
2823:
2818:
2813:
2808:
2803:
2798:
2793:
2788:
2783:
2778:
2773:
2768:
2763:
2758:
2753:
2748:
2743:
2738:
2733:
2728:
2723:
2718:
2713:
2708:
2703:
2698:
2688:
2683:
2673:
2668:
2663:
2658:
2653:
2648:
2643:
2638:
2633:
2628:
2623:
2618:
2613:
2603:
2598:
2593:
2588:
2583:
2578:
2573:
2568:
2563:
2558:
2553:
2548:
2543:
2538:
2533:
2528:
2523:
2518:
2513:
2508:
2503:
2498:
2401:
2391:
2331:
2101:
2086:
1735:
1529:
Krtička, J.; Kubát, J.; Krtičková, I. (2016). "Stellar wind models of subluminous hot stars".
1307:
971:
666:
363:
56:
3002:
2997:
1664:
1621:
1556:
1552:
1506:
1502:
1449:
1445:
1351:
1262:
1258:
1105:
1101:
993:
589:
470:
233:
31:
3528:
3077:
3072:
1029:
1025:
794:
602:
483:
312:
181:
81:
1122:
1617:
1347:
1303:
1209:
1182:
1152:
797:
secondary. The two stars have an orbit of 217 days and are separated by about 200
3520:
1813:
1763:
1021:
1013:
1005:
949:
674:
658:
377:
322:
298:
241:
221:
209:
3592:
3361:
3287:
2421:
1793:
1633:
1568:
1365:
1017:
1001:
997:
967:. It is isolated from the main stars of Perseus, but lies within its formal borders.
929:
884:
790:
755:
198:
157:
68:
1461:
1276:
1117:
814:
backwards by the modelled age of the system (57 million years) places it within the
3117:
1848:
1828:
1788:
1778:
1758:
1753:
1743:
1231:
T.; Ridgway, S. T.; Sturmann, J.; Sturmann, L.; Turner, N.; Farrington, C. (2015).
807:
798:
571:
544:
450:
423:
1650:
AEEA (Activities of
Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 10 日
1649:
1560:
1510:
1453:
1267:
1232:
1171:
VizieR On-line Data
Catalog: B/GCVS. Originally Published in: 2009yCat....102025S
1109:
825:. Due to its rapid rotation, the primary star has a polar radius about 5.5
3282:
3032:
3027:
2475:
2426:
2341:
1783:
1768:
917:
898:
894:
331:
147:
136:
94:
1625:
1198:
VizieR On-line Data
Catalog: V/50. Originally Published in: 1964BS....C......0H
909:
3502:
3217:
3151:
3062:
3037:
2992:
1843:
1833:
1823:
1773:
938:
762:
551:
463:
430:
360:
256:
169:
38:
3554:
3095:
2286:
2241:
2231:
2171:
2126:
2121:
2111:
2106:
2057:
2051:
2046:
2041:
2036:
2031:
2026:
2021:
2016:
2011:
2006:
2001:
1996:
1991:
1986:
1981:
1976:
1971:
1966:
1961:
1956:
1951:
1946:
1941:
1936:
1931:
1926:
1921:
1916:
1911:
1818:
1808:
1803:
1798:
1669:
3559:
3497:
3476:
3471:
3466:
3461:
3456:
3451:
3446:
3441:
3436:
3431:
3426:
3421:
3416:
3411:
3406:
3401:
3396:
3391:
3386:
3381:
3376:
3371:
3366:
3356:
3351:
3346:
3341:
3336:
3331:
3326:
3321:
3316:
3266:
3256:
3251:
3191:
3186:
3181:
3176:
3171:
3166:
3161:
3156:
3017:
3012:
2971:
2956:
2946:
2926:
2921:
2693:
2678:
2608:
2480:
2465:
2346:
2096:
2091:
2081:
2076:
1906:
1901:
1896:
1891:
1886:
1881:
1876:
1871:
1853:
873:
821:
The primary star rotates rapidly with a projected equatorial velocity of
651:
1290:
Wilson, R. E. (1953). "General
Catalogue of Stellar Radial Velocities".
3146:
3141:
3136:
953:
901:, being only about 3% as bright as the primary at visible wavelengths.
777:
3492:
3301:
3231:
3212:
1078:
Van
Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".
846:
717:
629:
564:
510:
443:
261:
1543:
1493:
1436:
1356:
1331:
1249:
3007:
1748:
1092:
908:
883:
star, with the outer layers stripped as it expanded away from the
776:
766:
290:
1726:
1311:
887:. Its luminosity is higher than expected for a normal 1.2
751:
637:
225:
213:
1673:
855:
1233:"Spectral and spatial imaging of the Be+sdO binary ϕ Persei"
1604:
Wagman, M. (August 1987). "Flamsteed's
Missing Stars".
3545:
3519:
3485:
3309:
3300:
3275:
3239:
3230:
3200:
3127:
3116:
3094:
2980:
2892:
2489:
2067:
1862:
1734:
1725:
1417:
1415:
1413:
1411:
1409:
1407:
1405:
1403:
1401:
869:star and has accreted material from its companion.
1380:"Sixth Catalog of Orbits of Visual Binary Stars"
1073:
1071:
1069:
1067:
1065:
992:, refers to an asterism consisting of φ Persei,
858:. The rapidly-spinning star is surrounded by a
1524:
1522:
1520:
1292:Carnegie Institute Washington D.C. Publication
1685:
1225:
1223:
1221:
1219:
1043:
1037:
981:
975:
8:
1665:HST Press release on the φ Per binary system
1580:
1578:
1473:
1471:
1134:
1132:
1130:
99:50° 41′ 19.4328″
1141:CDS/ADC Collection of Electronic Catalogues
832:and an equatorial radius of about 8.0
3542:
3516:
3306:
3236:
3124:
3091:
1731:
1692:
1678:
1670:
1542:
1492:
1435:
1355:
1266:
1248:
1091:
1050:the Second Star of Heaven's Great General
59:J2000
669: Persei, φ Per, Phi Per,
1061:
205:
1325:
1323:
1321:
1164:
1162:
18:
941:with eruptions and irregular fading.
872:The secondary star is also a class O
7:
1606:Journal for the History of Astronomy
854:nearly 15,000 times higher than the
920:for Phi Persei, adapted from Božić
217:
14:
956:in treating φ Persei as being in
16:Star in the constellation Perseus
3639:Gamma Cassiopeiae variable stars
3575:
3574:
1296:Carnegie Institution for Science
37:
30:
3629:Henry Draper Catalogue objects
781:φ Persei in optical light
48:Location of φ Persei (circled)
1:
3624:Bright Star Catalogue objects
3247:650 (Little Dumbbell Nebula)
1717:Perseus in Chinese astronomy
1531:Astronomy & Astrophysics
1481:Astronomy & Astrophysics
1237:Astronomy & Astrophysics
1561:10.1051/0004-6361/201628433
1511:10.1051/0004-6361/201628760
1454:10.1051/0004-6361/201731194
1268:10.1051/0004-6361/201425141
1044:
982:
240:4.54 ± 0.20
3665:
3614:B-type main-sequence stars
3498:UGC 2885 (Godzilla galaxy)
1626:10.1177/002182868701800305
1587:Astronomy and Astrophysics
1424:Astronomy and Astrophysics
1110:10.1051/0004-6361:20078357
1080:Astronomy and Astrophysics
793:primary of class B2 and a
3572:
3541:
3515:
3090:
1707:
1336:The Astrophysical Journal
1049:
1038:
976:
710:
664:
657:
537:
416:
411:
289:
285:
175:
168:
119:
53:
24:
3262:1499 (California Nebula)
1712:List of stars in Perseus
1701:Constellation of Perseus
3609:Perseus (constellation)
1553:2016A&A...593A.101K
1503:2016A&A...595A.132Z
1446:2018A&A...615A..30S
1259:2015A&A...577A..51M
1102:2007A&A...474..653V
1036:for φ Persei itself is
271:Absolute magnitude
106:Apparent magnitude
3634:Durchmusterung objects
989:Heaven's Great General
925:
810:and extrapolating its
782:
3018:HAT-P-29 (Muspelheim)
912:
852:bolometric luminosity
841:effective temperature
789:consisting of a blue
780:
761:, location about 720
346:Longitude of the node
3362:1175 (Peanut Galaxy)
3208:Alpha Persei Cluster
3013:HAT-P-15 (Berehynia)
1819:π (Gorgonea Secunda)
1123:Vizier catalog entry
1045:Tiān Dà Jiāng Jūn èr
1032:. Consequently, the
816:Alpha Persei cluster
787:spectroscopic binary
3547:Astronomical events
1849:ω (Gorgonea Quarta)
1824:ρ (Gorgonea Tertia)
1618:1987JHA....18..209W
1348:1998ApJ...493..440G
1304:1953GCRV..C......0W
1210:1995yCat.5050....0H
1183:2009yCat....102025S
1153:2002yCat.2237....0D
806:. Phi Persei is a
711:Database references
519:Rotational velocity
21:
3104:WASP-11b/HAT-P-10b
926:
860:circumstellar disk
783:
659:Other designations
220: −14.01
208: +24.59
158:Variable type
126:Spectral type
19:
3619:Hipparcos objects
3604:Flamsteed objects
3586:
3585:
3568:
3567:
3537:
3536:
3511:
3510:
3296:
3295:
3226:
3225:
3112:
3111:
3086:
3085:
983:Tiān Dà Jiāng Jūn
750:fourth-magnitude
729:
728:
3656:
3649:O-type subdwarfs
3578:
3577:
3543:
3517:
3307:
3237:
3125:
3092:
3058:NGC 1333 IRAS 4B
3053:NGC 1333 IRAS 4A
3048:NGC 1333 IRAS 2A
1732:
1694:
1687:
1680:
1671:
1652:
1648:
1644:
1638:
1637:
1601:
1595:
1594:
1582:
1573:
1572:
1546:
1526:
1515:
1514:
1496:
1475:
1466:
1465:
1439:
1419:
1396:
1395:
1393:
1391:
1386:on 1 August 2017
1382:. Archived from
1376:
1370:
1369:
1359:
1327:
1316:
1315:
1287:
1281:
1280:
1270:
1252:
1227:
1214:
1213:
1193:
1187:
1186:
1166:
1157:
1156:
1136:
1125:
1121:
1095:
1075:
1051:
1047:
1041:
1040:
985:
979:
978:
960:and gave it the
928:Phi Persei is a
849:
824:
649:
647:
368:
350:
325:
317:
219:
207:
120:Characteristics
115:
109:
89:
84:
54:Observation data
41:
34:
22:
3664:
3663:
3659:
3658:
3657:
3655:
3654:
3653:
3589:
3588:
3587:
3582:
3564:
3533:
3529:Perseus Cluster
3521:Galaxy clusters
3507:
3481:
3292:
3271:
3222:
3196:
3119:
3108:
3082:
3023:IRAS 04296+3429
2976:
2888:
2485:
2063:
1858:
1721:
1703:
1698:
1661:
1656:
1655:
1646:
1645:
1641:
1603:
1602:
1598:
1584:
1583:
1576:
1528:
1527:
1518:
1477:
1476:
1469:
1421:
1420:
1399:
1389:
1387:
1378:
1377:
1373:
1329:
1328:
1319:
1289:
1288:
1284:
1229:
1228:
1217:
1195:
1194:
1190:
1168:
1167:
1160:
1138:
1137:
1128:
1077:
1076:
1063:
1058:
947:
907:
893:
890:
882:
879:
868:
865:
844:
838:
835:
831:
828:
822:
804:
801:
775:
706:
645:
643:
603:Surface gravity
595:
592:
577:
574:
557:
554:
525: sin
484:Surface gravity
476:
473:
456:
453:
449:5.5 - 8.0
436:
433:
403:
401:
386:
384:
358:
343:
320:
313:Semi-major axis
310:
276:
260:(220 ± 10
259:
216:
192:+0.80 km/s
187:
182:Radial velocity
113:
104:
87:
82:Right ascension
80:
55:
49:
47:
46:
45:
44:
43:
42:
17:
12:
11:
5:
3662:
3660:
3652:
3651:
3646:
3641:
3636:
3631:
3626:
3621:
3616:
3611:
3606:
3601:
3591:
3590:
3584:
3583:
3573:
3570:
3569:
3566:
3565:
3563:
3562:
3557:
3551:
3549:
3539:
3538:
3535:
3534:
3532:
3531:
3525:
3523:
3513:
3512:
3509:
3508:
3506:
3505:
3500:
3495:
3489:
3487:
3483:
3482:
3480:
3479:
3474:
3469:
3464:
3459:
3454:
3449:
3444:
3439:
3434:
3429:
3424:
3419:
3414:
3409:
3404:
3399:
3394:
3389:
3384:
3379:
3374:
3369:
3364:
3359:
3354:
3349:
3344:
3339:
3334:
3329:
3324:
3319:
3313:
3311:
3304:
3298:
3297:
3294:
3293:
3291:
3290:
3285:
3279:
3277:
3273:
3272:
3270:
3269:
3264:
3259:
3254:
3249:
3243:
3241:
3234:
3228:
3227:
3224:
3223:
3221:
3220:
3215:
3210:
3204:
3202:
3198:
3197:
3195:
3194:
3189:
3184:
3179:
3174:
3169:
3164:
3159:
3154:
3149:
3144:
3139:
3133:
3131:
3122:
3114:
3113:
3110:
3109:
3107:
3106:
3100:
3098:
3088:
3087:
3084:
3083:
3081:
3080:
3075:
3073:PSR J0357+3205
3070:
3065:
3060:
3055:
3050:
3045:
3040:
3035:
3030:
3025:
3020:
3015:
3010:
3005:
3000:
2995:
2990:
2984:
2982:
2978:
2977:
2975:
2974:
2969:
2964:
2959:
2954:
2949:
2944:
2939:
2934:
2929:
2924:
2919:
2914:
2909:
2904:
2898:
2896:
2890:
2889:
2887:
2886:
2881:
2876:
2871:
2866:
2861:
2856:
2851:
2846:
2841:
2836:
2831:
2826:
2821:
2816:
2811:
2806:
2801:
2796:
2791:
2786:
2781:
2776:
2771:
2766:
2761:
2756:
2751:
2746:
2741:
2736:
2731:
2726:
2721:
2716:
2711:
2706:
2701:
2696:
2691:
2686:
2681:
2676:
2671:
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1659:External links
1657:
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1467:
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1371:
1357:10.1086/305113
1342:(1): 440–450.
1317:
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1188:
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1126:
1086:(2): 653–664.
1060:
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812:space velocity
802:
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785:Phi Persei is
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396:Semi-amplitude
392:
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378:Semi-amplitude
373:
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3308:
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3299:
3289:
3288:Wreath Nebula
3286:
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1363:
1358:
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1326:
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1322:
1318:
1313:
1309:
1305:
1301:
1297:
1293:
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1283:
1278:
1274:
1269:
1264:
1260:
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1242:
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1234:
1226:
1224:
1222:
1220:
1216:
1211:
1207:
1203:
1199:
1192:
1189:
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1180:
1176:
1172:
1165:
1163:
1159:
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1150:
1146:
1142:
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1127:
1124:
1119:
1115:
1111:
1107:
1103:
1099:
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1089:
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1081:
1074:
1072:
1070:
1068:
1066:
1062:
1055:
1053:
1046:
1035:
1031:
1027:
1023:
1019:
1018:56 Andromedae
1015:
1011:
1007:
1003:
1002:49 Andromedae
999:
998:51 Andromedae
995:
991:
990:
984:
973:
968:
966:
965:54 Andromedae
963:
959:
955:
951:
944:
942:
940:
936:
935:γ Cassiopeiae
931:
930:variable star
923:
919:
916:
911:
904:
902:
900:
896:
886:
885:main sequence
875:
870:
861:
857:
853:
848:
842:
823:440 km/s
819:
817:
813:
809:
805:
796:
792:
791:main sequence
788:
779:
772:
770:
768:
764:
760:
757:
756:constellation
753:
749:
745:
741:
740:φ Persei
737:
733:
725:
722:
720:
719:
715:
714:
709:
704:
701: 26670,
700:
696:
692:
689: 10516,
688:
684:
680:
676:
672:
671:54 Andromedae
668:
663:
660:
656:
653:
642:
640:
639:
635:
634:
631:
627:
625:
624:
620:
619:
616:
612:
610:
608:
604:
600:
599:
596:
587:
585:
582:
581:
578:
569:
567:
566:
562:
561:
558:
549:
547:
546:
542:
541:
536:
533:440 km/s
532:
530:
528:
524:
520:
516:
515:
512:
508:
506:
505:
501:
500:
497:
493:
491:
489:
485:
481:
480:
477:
468:
466:
465:
461:
460:
457:
448:
446:
445:
441:
440:
437:
428:
426:
425:
421:
420:
415:
410:
406:
397:
394:
393:
389:
380:
379:
375:
374:
370:
367:
365:
362:
357:
356:
352:
349:
347:
342:
341:
337:
335:
333:
329:
328:
324:
319:
316:
314:
309:
308:
305:126.6731 days
304:
302:
300:
296:
295:
292:
288:
284:
280:
278:
272:
268:
267:
263:
258:
254:
252:
251:
247:
246:
243:
239:
237:
235:
231:
230:
227:
223:
215:
211:
204:
202:
200:
199:Proper motion
196:
195:
191:
189:
183:
179:
178:
174:
171:
167:
164:
161:
159:
156:
155:
151:
149:
145:
144:
140:
138:
134:
133:
129:
127:
124:
123:
118:
114:(3.96 - 4.11)
111:
107:
103:
102:
98:
96:
93:
92:
86:
83:
79:
78:
75:
72:
70:
69:Constellation
67:
66:
62:
58:
52:
40:
33:
23:
3644:Binary stars
3068:PSR B0355+54
2428:
2056:
1838:
1647:(in Chinese)
1642:
1609:
1605:
1599:
1590:
1586:
1534:
1530:
1484:
1480:
1427:
1423:
1388:. Retrieved
1384:the original
1374:
1339:
1335:
1291:
1285:
1240:
1236:
1201:
1197:
1191:
1174:
1170:
1144:
1140:
1083:
1079:
1034:Chinese name
1014:τ Andromedae
1010:υ Andromedae
1006:χ Andromedae
994:γ Andromedae
987:
969:
964:
948:
927:
921:
871:
845:30,000
820:
808:runaway star
795:hot subdwarf
784:
743:
739:
736:Phi Per
735:
731:
730:
716:
705: 22554
693: 8068,
685: 2102,
636:
628:53,000
621:
606:
601:
583:
563:
543:
526:
522:
517:
509:29,300
502:
487:
482:
469:14,454
462:
442:
422:
395:
376:
359:
344:
330:
311:
297:
269:
248:
232:
197:
180:
130:B2Vep + sdO
3283:Barnard 203
3043:NGC 1333 13
3028:L1448-IRS2E
1390:29 December
1048:, English:
1030:δ Trianguli
1026:γ Trianguli
1022:β Trianguli
986:), meaning
962:designation
939:shell stars
918:light curve
905:Variability
899:ultraviolet
895:helium star
850:, it has a
839:. With an
763:light-years
748:class B2Vep
697: 496,
623:Temperature
588:6,310
504:Temperature
404:(secondary)
353:295.7°
332:Inclination
148:color index
137:color index
95:Declination
3593:Categories
3218:Trumpler 2
3096:Exoplanets
3063:NGC 1624-2
3038:LRLL 54361
1809:ξ (Menkib)
1744:α (Mirfak)
1612:(3): 212.
1593:: 235–257.
1544:1607.04445
1494:1702.07684
1437:1803.02379
1250:1503.03423
1056:References
915:blue-light
843:of nearly
744:φ Per
732:Phi Persei
681: 57,
605:(log
584:Luminosity
550:1.14
494:4.46
486:(log
464:Luminosity
371:2456110.03
361:Periastron
338:77.6°
321:5.89
170:Astrometry
3555:SN 2006gy
3503:4C +37.11
2993:BD+48 740
2988:BD+31 643
1864:Flamsteed
1789:κ (Misam)
1774:η (Miram)
1749:β (Algol)
1634:118445625
1569:118390374
1366:121635926
1093:0708.1752
958:Andromeda
952:followed
950:Flamsteed
677:+49°444,
613:4.2
570:1.3
429:9.6
407:81.3 km/s
390:9.97 km/s
387:(primary)
108: (V)
20:φ Persei
3580:Category
3560:Perseids
3302:Galaxies
3120:clusters
3033:LkHα 101
2069:Variable
1814:ο (Atik)
1537:: A101.
1487:: A132.
1462:59471417
1312:54001336
1277:16766856
1118:18759600
892:☉
881:☉
874:subdwarf
867:☉
837:☉
830:☉
803:☉
594:☉
576:☉
556:☉
475:☉
455:☉
435:☉
273: (M
250:Distance
234:Parallax
3232:Nebulae
3142:884 (χ)
3137:869 (h)
3003:G 95-57
2998:G 38-29
2609:918 (k)
1614:Bibcode
1549:Bibcode
1499:Bibcode
1442:Bibcode
1430:: A30.
1344:Bibcode
1300:Bibcode
1255:Bibcode
1243:: A51.
1206:Bibcode
1179:Bibcode
1149:Bibcode
1098:Bibcode
972:Chinese
954:Ptolemy
937:-type,
759:Perseus
754:in the
746:) is a
412:Details
74:Perseus
61:Equinox
3493:IC 310
3213:IC 348
2429:61 And
2427:V520 (
2047:58 (e)
2042:57 (m)
2022:53 (d)
2017:52 (f)
2002:48 (c)
1997:43 (A)
1992:42 (n)
1987:40 (o)
1972:32 (l)
1632:
1567:
1460:
1364:
1310:
1275:
1116:
945:Naming
924:(1995)
922:et al.
773:System
718:SIMBAD
650:
565:Radius
444:Radius
299:Period
152:−0.04
141:−0.92
63:J2000
3486:Other
3276:Other
3201:Other
3008:GD 61
2981:Other
2972:29587
2967:26702
2962:25329
2957:23596
2952:23301
2947:22781
2942:21684
2937:17605
2932:17245
2927:17092
2922:16760
2917:16691
2912:14434
2907:14433
2902:13519
2481:V1024
2058:1 Aur
1907:9 (i)
1887:4 (g)
1736:Bayer
1727:Stars
1630:S2CID
1565:S2CID
1539:arXiv
1489:arXiv
1458:S2CID
1432:arXiv
1362:S2CID
1273:S2CID
1245:arXiv
1114:S2CID
1088:arXiv
1039:天大將軍二
767:Earth
765:from
364:epoch
291:Orbit
281:−3.11
218:Dec.:
163:γ Cas
112:4.06
57:Epoch
3477:1334
3472:1294
3467:1293
3462:1283
3457:1282
3452:1281
3447:1279
3442:1278
3437:1277
3432:1275
3427:1274
3422:1273
3417:1272
3412:1271
3407:1270
3402:1268
3397:1267
3392:1265
3387:1264
3382:1260
3377:1259
3372:1250
3367:1198
3357:1169
3352:1167
3347:1161
3342:1160
3337:1086
3332:1077
3327:1058
3322:1023
3317:1003
3267:1579
3257:1491
3252:1333
3192:1624
3187:1545
3182:1528
3177:1513
3172:1444
3167:1342
3162:1285
3157:1220
3152:1039
3118:Star
3078:WR 4
2884:1514
2879:1500
2874:1493
2869:1489
2864:1482
2859:1424
2854:1419
2849:1390
2844:1371
2839:1344
2834:1337
2829:1333
2824:1330
2819:1301
2814:1286
2809:1234
2804:1226
2799:1215
2794:1207
2789:1198
2784:1197
2779:1191
2774:1176
2769:1164
2764:1160
2759:1141
2754:1133
2749:1130
2744:1127
2739:1113
2734:1097
2729:1074
2724:1059
2719:1056
2714:1051
2709:1047
2704:1041
2699:1037
2694:1034
2689:1019
2684:1001
2476:V718
2471:V621
2466:V576
2461:V575
2456:V573
2451:V572
2446:V551
2441:V545
2436:V521
2422:V518
2417:V509
2412:V505
2407:V492
2402:V490
2397:V480
2392:V473
2387:V472
2382:V471
2377:V461
2372:V459
2367:V440
2362:V432
2357:V423
2352:V400
2347:V396
2342:V392
2337:V386
2332:V380
2327:V376
2322:V361
2317:V357
2312:V356
2307:V351
1392:2016
1308:LCCN
1202:5050
1145:2237
1052:.).
1028:and
977:天大將軍
752:star
724:data
545:Mass
424:Mass
146:B−V
135:U−B
3310:NGC
3240:NGC
3147:957
3129:NGC
2679:991
2674:986
2669:979
2664:975
2659:973
2654:969
2649:966
2644:964
2639:956
2634:950
2629:949
2624:930
2619:923
2614:920
2604:894
2599:890
2594:886
2589:885
2584:876
2579:865
2574:864
2569:849
2564:846
2559:842
2554:831
2549:820
2544:810
2539:792
2534:787
2529:641
2524:621
2519:540
2514:538
2509:529
2504:526
2499:470
1622:doi
1591:304
1557:doi
1535:593
1507:doi
1485:595
1450:doi
1428:615
1352:doi
1340:493
1263:doi
1241:577
1106:doi
1084:474
970:In
856:Sun
703:SAO
699:PPM
691:HIP
679:FK5
652:Myr
638:Age
615:cgs
496:cgs
366:(T)
348:(Ω)
334:(i)
323:mas
315:(a)
301:(P)
242:mas
236:(π)
222:mas
210:mas
206:RA:
201:(μ)
3595::
2894:HD
2491:HR
2302:LX
2297:KW
2292:KT
2287:KS
2282:KP
2277:IZ
2272:IX
2267:IW
2262:IU
2257:IQ
2252:IP
2247:IK
2242:GK
2237:FO
2232:DY
2227:DM
2222:BM
2217:AX
2212:AW
2207:AS
2202:AR
2197:AG
2192:AB
2187:YZ
2182:XZ
2177:XY
2172:XX
2167:VX
2162:UY
2157:UX
2152:UV
2147:TZ
2142:SV
2137:SU
2132:ST
2127:RY
2122:RW
2117:RV
2112:RT
2107:RS
2052:59
2037:56
2032:55
2027:54
2012:50
2007:49
1982:36
1977:34
1967:31
1962:30
1957:29
1952:24
1947:21
1942:20
1937:17
1932:16
1927:14
1922:12
1917:11
1912:10
1628:.
1620:.
1610:18
1608:.
1589:.
1577:^
1563:.
1555:.
1547:.
1533:.
1519:^
1505:.
1497:.
1483:.
1470:^
1456:.
1448:.
1440:.
1426:.
1400:^
1360:.
1350:.
1338:.
1334:.
1320:^
1306:.
1298:.
1294:.
1271:.
1261:.
1253:.
1239:.
1235:.
1218:^
1204:.
1200:.
1177:.
1173:.
1161:^
1147:.
1143:.
1129:^
1112:.
1104:.
1096:.
1082:.
1064:^
1024:,
1020:,
1016:,
1012:,
1008:,
1004:,
1000:,
996:,
974:,
913:A
818:.
769:.
742:,
738:,
695:HR
687:HD
683:GC
675:BD
673:,
644:57
398:(K
381:(K
262:pc
257:ly
226:yr
214:yr
184:(R
2431:)
2102:Z
2097:X
2092:V
2087:U
2082:T
2077:S
1902:8
1897:7
1892:5
1882:3
1877:2
1872:1
1854:b
1844:ψ
1839:φ
1834:τ
1829:σ
1804:ν
1799:μ
1794:λ
1784:ι
1779:θ
1769:ζ
1764:ε
1759:δ
1754:γ
1693:e
1686:t
1679:v
1636:.
1624::
1616::
1571:.
1559::
1551::
1541::
1513:.
1509::
1501::
1491::
1464:.
1452::
1444::
1434::
1394:.
1368:.
1354::
1346::
1314:.
1302::
1279:.
1265::
1257::
1247::
1212:.
1208::
1185:.
1181::
1175:1
1155:.
1151::
1120:.
1108::
1100::
1090::
1042:(
980:(
889:M
878:M
864:M
847:K
834:R
827:R
800:R
734:(
667:φ
648:9
646:±
630:K
609:)
607:g
591:L
573:R
553:M
538:B
529:)
527:i
523:v
521:(
511:K
490:)
488:g
472:L
452:R
432:M
417:A
402:)
400:2
385:)
383:1
277:)
275:V
264:)
224:/
212:/
188:)
186:v
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