3375:
980:
46:
3435:
3337:
1810:
58:
3399:
3423:
1820:
3387:
3411:
3348:
220:
as a small galaxy. As a quasi-star cools over time, its outer envelope would become transparent, until further cooling to a limiting temperature of 4,000 K (3,730 °C). This limiting temperature would mark the end of the quasi-star's life since there is no
193:, creating an equilibrium similar to the one that supports modern fusion-based stars. Quasi-stars would have had a short maximum lifespan, approximately 7 million years, during which the core black hole would have grown to about 1,000–10,000 solar masses (2
161:
with tens of thousands of solar masses. Formation of quasi-stars could only happen early in the development of the
Universe before hydrogen and helium were contaminated by heavier elements; thus, they may have been very massive
541:
Schleicher, Dominik R. G.; Palla, Francesco; Ferrara, Andrea; Galli, Daniele; Latif, Muhammad (25 May 2013). "Massive black hole factories: Supermassive and quasi-star formation in primordial halos".
141:, where the outer layers of the protostar are massive enough to absorb the resulting burst of energy without being blown away or falling into the black hole, as occurs with modern
3188:
1705:
216:
Quasi-stars are predicted to have had surface temperatures higher than 10,000 K (9,700 °C). At these temperatures, each one would be about as
297:
1061:
841:
1066:
1785:
1442:
1380:
1206:
1106:
667:
Czerny, Bozena; Janiuk, Agnieszka; Sikora, Marek; Lasota, Jean-Pierre (2012). "Quasi-Star Jets as
Unidentified Gamma-Ray Sources".
369:
3220:
883:
3195:
2514:
1422:
1511:
1506:
3374:
1391:
2907:
1427:
1223:
3200:
2837:
2821:
1856:
1649:
1330:
969:
716:"Light or heavy supermassive black hole seeds: The role of internal rotation in the fate of supermassive stars"
3247:
3114:
1417:
1292:
395:
113:
at its core. They were first proposed in the 1960s and have since provided valuable insights into the early
3230:
3181:
3156:
2449:
1823:
1335:
1238:
1026:
226:
202:
1345:
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1594:
210:
179:
2534:
257:
3365:
3235:
3166:
3136:
1325:
1277:
1260:
959:
269:
185:
Once the black hole had formed at the protostar's core, it would continue generating a large amount of
3242:
3119:
3096:
2678:
2127:
2122:
2117:
2112:
2107:
2102:
1780:
1282:
1196:
944:
876:
189:
from the infall of stellar material. This constant outburst of energy would counteract the force of
2385:
2259:
1894:
1457:
239:
225:
at or below this limiting temperature. The object would then quickly dissipate, leaving behind the
3161:
2912:
2711:
2621:
2581:
2563:
2489:
2060:
1986:
1634:
1170:
1133:
1036:
1031:
949:
242: – Accumulation of particles into a massive object by gravitationally attracting more matter
222:
206:
122:
94:
3322:
3302:
3074:
3069:
2967:
2862:
2811:
2616:
2606:
2279:
2077:
2045:
1936:
1919:
1664:
1552:
1537:
1396:
1089:
903:
3176:
3146:
3141:
3131:
3059:
2847:
2013:
1542:
1355:
1099:
954:
50:
2294:
564:
248: – Structure formed by diffuse material in orbital motion around a massive central body
3455:
3317:
3215:
3205:
3054:
3022:
2816:
2611:
2596:
1909:
1813:
1521:
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1376:
1304:
1272:
1116:
924:
869:
811:
686:
622:
560:
505:
443:
340:
121:. Although they have not been observed, they are considered to be a possible progenitor of
420:
Ball, Warrick H.; Tout, Christopher A.; Żytkow, Anna N.; Eldridge, John J. (1 July 2011).
8:
3460:
3427:
2777:
2760:
2431:
2333:
2156:
1644:
1619:
1589:
1547:
1501:
1138:
1004:
999:
929:
373:
2917:
815:
690:
626:
509:
447:
422:"The structure and evolution of quasi-stars: The structure and evolution of quasi-stars"
344:
3415:
3403:
3312:
3273:
3225:
3210:
3124:
3064:
2987:
2897:
2867:
2857:
2801:
2723:
2414:
2050:
1849:
1478:
1350:
1255:
1046:
1014:
979:
939:
934:
801:
764:
727:
702:
676:
653:
640:
612:
576:
550:
523:
495:
433:
330:
20:
698:
3263:
2688:
2661:
2641:
2441:
2225:
2213:
2040:
2020:
1974:
1956:
1924:
1624:
1614:
1609:
1309:
1297:
1250:
1191:
1160:
1150:
1084:
824:
789:
706:
644:
635:
600:
580:
518:
483:
456:
421:
353:
318:
158:
79:
2748:
527:
3391:
3091:
3044:
2994:
2982:
2960:
2955:
2882:
2842:
2789:
2571:
2494:
2469:
2363:
2284:
2008:
1969:
1775:
1735:
1483:
1432:
1287:
1201:
994:
964:
819:
774:
737:
694:
630:
599:
Ball, Warrick H.; Tout, Christopher A.; Żytkow, Anna N.; Eldridge, John J. (2011).
568:
513:
451:
348:
317:
Ball, Warrick H.; Tout, Christopher A.; Żytkow, Anna N.; Eldridge, John J. (2011).
167:
154:
572:
3278:
3081:
2950:
2794:
2765:
2706:
2701:
2576:
2304:
2269:
2203:
2149:
2144:
2089:
1899:
1795:
1745:
1720:
1516:
1360:
1267:
1233:
1145:
97:. They are thought to have lived around 7-10 million years due to their immense
3439:
3379:
3340:
3106:
2945:
2772:
2743:
2718:
2651:
2340:
2208:
2094:
1996:
1886:
1876:
1710:
1695:
1462:
1401:
1245:
919:
245:
186:
163:
102:
32:
853:
652:
Ball, Warrick H. (2012). "Quasi-stars and the Schönberg-Chandrasekhar limit".
3449:
3292:
3086:
3049:
3017:
2892:
2601:
2424:
2395:
2373:
1991:
1964:
1941:
1842:
1770:
1690:
1218:
1213:
399:
302:
45:
779:
752:
742:
715:
3352:
3027:
2977:
2972:
2872:
2755:
2738:
2696:
2666:
2656:
2591:
2474:
2419:
2400:
2380:
2358:
2350:
2193:
2186:
2025:
1946:
1929:
1725:
1599:
1567:
1175:
1094:
263:
753:"Modelling supermassive primordial stars with <SCP>mesa</SCP>"
19:"Black hole star" redirects here. For black holes created from stars, see
3268:
2940:
2932:
2922:
2902:
2877:
2806:
2728:
2484:
2459:
2454:
2368:
2328:
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2254:
2237:
2232:
1904:
1765:
1715:
1669:
1572:
1447:
1386:
1111:
1019:
118:
28:
2852:
2549:
2499:
2479:
2464:
2316:
2220:
2198:
2176:
2171:
2035:
1755:
1685:
1654:
1582:
1577:
1562:
1228:
1155:
1056:
892:
849:
217:
146:
138:
110:
87:
3434:
842:"Quasi-Stars: Black Holes at the Core of the Universe's Largest Stars"
57:
3039:
2887:
2671:
2636:
2631:
2626:
2586:
2539:
2529:
2323:
2299:
2274:
2181:
2132:
2065:
2055:
2030:
2003:
1979:
1914:
1790:
1437:
1340:
1128:
1123:
751:
Herrington, Nicholas P.; Whalen, Daniel J.; Woods, Tyrone E. (2023).
175:
171:
142:
134:
24:
481:
3032:
2733:
2407:
2166:
2139:
1700:
1659:
1557:
769:
732:
114:
62:
806:
681:
658:
617:
555:
500:
438:
335:
157:
drawing in enormous amounts of gas via gravity, which can produce
3307:
2782:
2544:
2311:
2264:
2247:
2242:
2161:
1740:
790:"A lower limit on the halo mass to form supermassive black holes"
251:
190:
3297:
3285:
2504:
2390:
1760:
1750:
1730:
1452:
1051:
1041:
106:
39:
861:
484:"Quasi-stars: accreting black holes inside massive envelopes"
49:
Size comparison of a hypothetical quasi-star to some of the
2646:
1865:
540:
396:"Cooking up supermassive black holes in the early universe"
98:
90:
83:
3347:
133:
A quasi-star would have resulted from the core of a large
3012:
1834:
788:
Dotan, Calanit; Rossi, Elena M.; Shaviv, Nir J. (2011).
666:
482:
Begelman, Mitch; Rossi, Elena; Armitage, Philip (2008).
16:
Hypothetical early-universe star with a black hole core
598:
419:
316:
3363:
750:
27:. For types of stars denser than neutron stars, see
370:"Zeroing In on How Supermassive Black Holes Formed"
153:10 kg). Quasi-stars may have also formed from
298:"Biggest black holes may grow inside 'quasistars'"
38:Not to be confused with a quasi-stellar object or
794:Monthly Notices of the Royal Astronomical Society
757:Monthly Notices of the Royal Astronomical Society
720:Monthly Notices of the Royal Astronomical Society
605:Monthly Notices of the Royal Astronomical Society
426:Monthly Notices of the Royal Astronomical Society
323:Monthly Notices of the Royal Astronomical Society
205:have been suggested as the progenitors of modern
3447:
787:
855:Black Hole Star – The Star That Shouldn't Exist
145:. Such a star would have to be at least 1,000
1850:
877:
713:
601:"The structure and evolution of quasi-stars"
319:"The structure and evolution of quasi-stars"
101:. Unlike modern stars, which are powered by
393:
128:
1857:
1843:
1443:Magnetospheric eternally collapsing object
884:
870:
848:
714:Fiacconi, Davide; Rossi, Elena M. (2017).
367:
823:
805:
778:
768:
741:
731:
680:
657:
634:
616:
554:
517:
499:
455:
437:
387:
368:Saplakoglu, Yasemin (29 September 2017).
361:
352:
334:
295:
254: – Hypothetical type of neutron star
23:. For stars that become black holes, see
291:
289:
287:
266: – Collapsed core of a massive star
117:, galaxy formation, and the behavior of
109:would come from material falling into a
56:
44:
477:
475:
473:
471:
469:
467:
296:Battersby, Stephen (29 November 2007).
3448:
394:Johnson-Goh, Mara (20 November 2017).
1838:
865:
284:
260: – Hypothetical hybrid star type
31:. For the 1994 Soundgarden song, see
1819:
651:
534:
464:
310:
211:the one in the center of the Galaxy
93:that may have existed early in the
13:
591:
272: – High-mass black hole seeds
14:
3477:
834:
3433:
3421:
3409:
3397:
3385:
3373:
3346:
3336:
3335:
1818:
1809:
1808:
1107:Tolman–Oppenheimer–Volkoff limit
978:
825:10.1111/j.1365-2966.2011.19461.x
636:10.1111/j.1365-2966.2011.18591.x
519:10.1111/j.1365-2966.2008.13344.x
457:10.1111/j.1365-2966.2011.18591.x
354:10.1111/j.1365-2966.2011.18591.x
1224:Innermost stable circular orbit
891:
105:in their cores, a quasi-star's
1650:Timeline of black hole physics
413:
166:stars. Such stars would dwarf
1:
3248:Timeline of stellar astronomy
1418:Nonsingular black hole models
277:
203:intermediate-mass black holes
543:Astronomy & Astrophysics
227:intermediate mass black hole
7:
2908:Hertzsprung–Russell diagram
1640:Rossi X-ray Timing Explorer
1605:Hypercompact stellar system
1595:Gamma-ray burst progenitors
699:10.1088/2041-8205/755/1/L15
573:10.1051/0004-6361/201321949
232:
61:A quasi-star rendered with
10:
3482:
2822:Kelvin–Helmholtz mechanism
1326:Black hole complementarity
1293:Bousso's holographic bound
1278:Quasi-periodic oscillation
976:
970:Malament–Hogarth spacetime
270:Direct collapse black hole
180:largest known modern stars
37:
18:
3331:
3256:
3105:
3003:
2931:
2830:
2687:
2562:
2440:
2349:
2085:
2076:
1955:
1885:
1872:
1864:
1804:
1678:
1530:
1492:
1471:
1410:
1369:
1318:
1197:Gravitational singularity
1184:
1077:
987:
912:
899:
669:The Astrophysical Journal
3201:With multiple exoplanets
1781:PSO J030947.49+271757.31
1706:SDSS J150243.09+111557.3
1239:Blandford–Znajek process
240:Accretion (astrophysics)
207:supermassive black holes
129:Formation and properties
123:supermassive black holes
1987:Asymptotic giant branch
1037:Active galactic nucleus
565:2013A&A...558A..59S
223:hydrostatic equilibrium
95:history of the Universe
3323:Tidal disruption event
2812:Circumstellar envelope
2046:Luminous blue variable
1665:Tidal disruption event
1635:Supermassive dark star
1553:Black holes in fiction
1538:Outline of black holes
1171:Supermassive dark star
1090:Gravitational collapse
65:
54:
2848:Effective temperature
1543:Black Hole Initiative
1356:Holographic principle
780:10.1093/mnras/stad572
743:10.1093/mnras/stw2505
60:
48:
3318:Planet-hosting stars
3196:With resolved images
3167:Historical brightest
3097:Photometric-standard
3023:Solar radio emission
2817:Eddington luminosity
2597:Triple-alpha process
2535:Thorne–Żytkow object
1910:Young stellar object
1346:Final parsec problem
1305:Schwarzschild radius
852:(15 December 2022),
258:Thorne–Żytkow object
3142:Highest temperature
2913:Color–color diagram
2778:Protoplanetary disk
2582:Proton–proton chain
2260:Chemically peculiar
1645:Superluminal motion
1620:Population III star
1590:Gravitational waves
1548:Black hole starship
1331:Information paradox
816:2011MNRAS.417.3035D
691:2012ApJ...755L..15C
627:2011MNRAS.414.2751B
510:2008MNRAS.387.1649B
448:2011MNRAS.414.2751B
374:Scientific American
345:2011MNRAS.414.2751B
201:10 kg). These
51:largest known stars
3466:Hypothetical stars
3147:Lowest temperature
2898:Photometric system
2868:Absolute magnitude
2802:Circumstellar dust
2415:Stellar black hole
2051:Stellar population
1937:Herbig–Haro object
1479:Optical black hole
1392:Reissner–Nordström
1351:Firewall (physics)
1256:Gravitational lens
159:supermassive stars
137:collapsing into a
66:
55:
21:Stellar black hole
3361:
3360:
3264:Substellar object
3243:Planetary nebulae
2662:Luminous red nova
2572:Deuterium burning
2558:
2557:
2041:Instability strip
2021:Wolf-Rayet nebula
1975:Horizontal branch
1920:Pre-main-sequence
1832:
1831:
1625:Supermassive star
1615:Naked singularity
1610:Membrane paradigm
1336:Cosmic censorship
1310:Spaghettification
1298:Immirzi parameter
1251:Hawking radiation
1192:Astrophysical jet
1161:Supermassive star
1151:Binary black hole
1085:Stellar evolution
1027:Intermediate-mass
178:, four among the
155:dark matter halos
80:hypothetical type
3473:
3438:
3437:
3426:
3425:
3424:
3414:
3413:
3412:
3402:
3401:
3400:
3390:
3389:
3388:
3378:
3377:
3369:
3353:Stars portal
3351:
3350:
3339:
3338:
2995:Planetary system
2918:Strömgren sphere
2790:Asteroseismology
2511:Black hole star
2083:
2082:
2009:Planetary nebula
1970:Red-giant branch
1859:
1852:
1845:
1836:
1835:
1822:
1821:
1812:
1811:
1484:Sonic black hole
1433:Dark-energy star
1288:Bekenstein bound
1273:M–sigma relation
1202:Ring singularity
982:
886:
879:
872:
863:
862:
858:
845:
829:
827:
809:
800:(4): 3035–3046.
784:
782:
772:
747:
745:
735:
726:(2): 2259–2269.
710:
684:
663:
661:
648:
638:
620:
611:(3): 2751–2762.
585:
584:
558:
538:
532:
531:
521:
503:
494:(4): 1649–1659.
479:
462:
461:
459:
441:
432:(3): 2751–2762.
417:
411:
410:
408:
406:
391:
385:
384:
382:
380:
365:
359:
358:
356:
338:
329:(3): 2751–2762.
314:
308:
307:
293:
200:
196:
168:VY Canis Majoris
152:
3481:
3480:
3476:
3475:
3474:
3472:
3471:
3470:
3446:
3445:
3444:
3432:
3422:
3420:
3410:
3408:
3398:
3396:
3386:
3384:
3372:
3364:
3362:
3357:
3345:
3327:
3252:
3221:Milky Way novae
3157:Smallest volume
3101:
3082:Radial velocity
3005:
2999:
2951:Common envelope
2927:
2826:
2795:Helioseismology
2766:Bipolar outflow
2707:Microturbulence
2702:Convection zone
2683:
2577:Lithium burning
2564:Nucleosynthesis
2554:
2436:
2345:
2072:
1951:
1900:Molecular cloud
1881:
1868:
1863:
1833:
1828:
1800:
1776:ULAS J1342+0928
1736:SDSS J0849+1114
1721:Phoenix Cluster
1674:
1526:
1488:
1467:
1406:
1365:
1361:No-hair theorem
1314:
1268:Bondi accretion
1234:Penrose process
1180:
1146:Gamma-ray burst
1073:
983:
974:
960:Direct collapse
908:
895:
890:
840:
837:
832:
594:
592:Further reading
589:
588:
539:
535:
480:
465:
418:
414:
404:
402:
392:
388:
378:
376:
366:
362:
315:
311:
294:
285:
280:
275:
235:
198:
194:
150:
131:
76:black hole star
43:
36:
17:
12:
11:
5:
3479:
3469:
3468:
3463:
3458:
3443:
3442:
3430:
3418:
3406:
3394:
3382:
3359:
3358:
3356:
3355:
3343:
3332:
3329:
3328:
3326:
3325:
3320:
3315:
3310:
3305:
3300:
3295:
3290:
3289:
3288:
3283:
3282:
3281:
3276:
3260:
3258:
3254:
3253:
3251:
3250:
3245:
3240:
3239:
3238:
3233:
3223:
3218:
3213:
3208:
3203:
3198:
3193:
3192:
3191:
3186:
3185:
3184:
3174:
3169:
3164:
3159:
3154:
3152:Largest volume
3149:
3144:
3139:
3129:
3128:
3127:
3122:
3111:
3109:
3103:
3102:
3100:
3099:
3094:
3089:
3084:
3079:
3078:
3077:
3072:
3067:
3057:
3052:
3047:
3042:
3037:
3036:
3035:
3030:
3025:
3020:
3009:
3007:
3001:
3000:
2998:
2997:
2992:
2991:
2990:
2985:
2980:
2970:
2965:
2964:
2963:
2958:
2953:
2948:
2937:
2935:
2929:
2928:
2926:
2925:
2920:
2915:
2910:
2905:
2900:
2895:
2890:
2885:
2880:
2875:
2870:
2865:
2863:Magnetic field
2860:
2855:
2850:
2845:
2840:
2834:
2832:
2828:
2827:
2825:
2824:
2819:
2814:
2809:
2804:
2799:
2798:
2797:
2787:
2786:
2785:
2780:
2773:Accretion disk
2770:
2769:
2768:
2763:
2753:
2752:
2751:
2749:Alfvén surface
2746:
2744:Stellar corona
2741:
2736:
2731:
2721:
2719:Radiation zone
2716:
2715:
2714:
2709:
2699:
2693:
2691:
2685:
2684:
2682:
2681:
2676:
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2099:Main sequence
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2078:Classification
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2068:
2063:
2053:
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2014:Protoplanetary
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1796:Swift J1644+57
1793:
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1758:
1753:
1748:
1746:MS 0735.6+7421
1743:
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1723:
1718:
1713:
1711:Sagittarius A*
1708:
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1290:
1285:
1283:Thermodynamics
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1270:
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1248:
1246:Accretion disk
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932:
927:
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920:BTZ black hole
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844:. 16 May 2020.
836:
835:External links
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246:Accretion disk
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187:radiant energy
164:Population III
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103:nuclear fusion
33:Black Hole Sun
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3050:Constellation
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3018:Solar eclipse
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3004:Earth-centric
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2602:Alpha process
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2383:
2382:
2379:
2375:
2374:Helium planet
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2370:
2367:
2365:
2364:Parker's star
2362:
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2295:Lambda Boötis
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2061:Superluminous
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1965:Main sequence
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1954:
1948:
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1942:Hayashi track
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1696:XTE J1118+480
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1377:Schwarzschild
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1220:
1219:Photon sphere
1217:
1215:
1214:Event horizon
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1139:Related links
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1117:Related links
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3428:Solar System
3216:White dwarfs
3206:Brown dwarfs
3189:Most distant
3137:Most massive
3115:Proper names
3075:Photographic
3028:Solar System
3006:observations
2933:Star systems
2756:Stellar wind
2739:Chromosphere
2712:Oscillations
2592:Helium flash
2522:
2442:Hypothetical
2420:X-ray binary
2359:Compact star
2194:Bright giant
1947:Henyey track
1925:Herbig Ae/Be
1726:PKS 1302-102
1629:
1600:Gravity well
1568:Compact star
1522:Microquasars
1507:Most massive
1411:Alternatives
1176:X-ray binary
1165:
1095:Neutron star
1032:Supermassive
1009:Hawking star
950:Supermassive
854:
797:
793:
760:
756:
723:
719:
672:
668:
608:
604:
546:
542:
536:
491:
487:
429:
425:
415:
403:. Retrieved
389:
377:. Retrieved
363:
326:
322:
312:
301:
264:Neutron star
215:
184:
147:solar masses
132:
75:
71:
69:
67:
3456:Black holes
3416:Outer space
3404:Spaceflight
3269:Brown dwarf
3045:Circumpolar
2923:Kraft break
2903:Color index
2878:Metallicity
2838:Designation
2807:Cosmic dust
2729:Photosphere
2495:Dark-energy
2470:Electroweak
2455:Black dwarf
2386:Radio-quiet
2369:White dwarf
2255:White dwarf
1905:Bok globule
1716:Centaurus A
1670:Planet Nine
1573:Exotic star
1502:Black holes
1448:Planck star
1397:Kerr–Newman
1112:White dwarf
1062:Radio-Quiet
1020:Microquasar
893:Black holes
763:: 463–473.
119:black holes
29:Exotic star
3461:Star types
3450:Categories
3231:Candidates
3226:Supernovae
3211:Red dwarfs
3070:Extinction
2858:Kinematics
2853:Luminosity
2831:Properties
2724:Atmosphere
2622:Si burning
2612:Ne burning
2550:White hole
2523:Quasi-star
2450:Blue dwarf
2305:Technetium
2221:Hypergiant
2199:Supergiant
1766:Q0906+6930
1756:Hercules A
1686:Cygnus X-1
1655:White hole
1630:Quasi-star
1583:Preon star
1578:Quark star
1563:Big Bounce
1423:Black star
1381:Derivation
1229:Ergosphere
1185:Properties
1166:Quasi-star
1156:Quark star
1067:Radio-Loud
955:Primordial
945:Kugelblitz
850:Kurzgesagt
770:2208.00008
733:1604.03936
675:(1): L15.
278:References
143:supernovae
139:black hole
111:black hole
72:quasi-star
3392:Astronomy
3162:Brightest
3060:Magnitude
3040:Pole star
2961:Symbiotic
2956:Eclipsing
2888:Starlight
2689:Structure
2679:Supernova
2672:Micronova
2667:Recurrent
2652:Symbiotic
2637:p-process
2632:r-process
2627:s-process
2617:O burning
2607:C burning
2587:CNO cycle
2530:Gravastar
2066:Hypernova
2056:Supernova
2031:Dredge-up
2004:Blue loop
1997:super-AGB
1980:Red clump
1957:Evolution
1915:Protostar
1895:Accretion
1887:Formation
1791:AT2018hyz
1438:Gravastar
1428:Dark star
1261:Microlens
1134:Hypernova
1129:Micronova
1124:Supernova
1078:Formation
807:1107.3562
707:113397287
682:1207.1560
659:1207.5972
645:119239346
618:1102.5098
581:119197147
556:1305.5923
501:0711.4078
439:1102.5098
336:1102.5098
176:RSGC1-F01
172:Mu Cephei
135:protostar
25:Supernova
3341:Category
3236:Remnants
3132:Extremes
3092:Parallax
3065:Apparent
3055:Asterism
3033:Sunlight
2983:Globular
2968:Multiple
2893:Variable
2883:Rotation
2843:Dynamics
2734:Starspot
2408:Magnetar
2351:Remnants
2167:Subgiant
2140:Subdwarf
1992:post-AGB
1814:Category
1701:A0620-00
1660:Wormhole
1558:Big Bang
1458:Fuzzball
1341:ER = EPR
1207:Theorems
1005:Electron
1000:Extremal
930:Rotating
528:12044015
233:See also
218:luminous
209:such as
115:universe
88:luminous
63:Celestia
3440:Science
3380:Physics
3366:Portals
3308:Gravity
3257:Related
3177:Nearest
3125:Chinese
2973:Cluster
2946:Contact
2783:Proplyd
2657:Remnant
2545:Blitzar
2519:Hawking
2475:Strange
2425:Burster
2381:Neutron
2334:Extreme
2285:He-weak
1930:T Tauri
1824:Commons
1786:P172+18
1741:TON 618
1679:Notable
1531:Related
1517:Quasars
1512:Nearest
1472:Analogs
1402:Hayward
1370:Metrics
1015:Stellar
940:Virtual
935:Charged
904:Outline
812:Bibcode
687:Bibcode
623:Bibcode
561:Bibcode
549:: A59.
506:Bibcode
444:Bibcode
405:8 April
379:8 April
341:Bibcode
252:Blitzar
191:gravity
84:massive
78:) is a
3298:Galaxy
3286:Planet
3274:Desert
3182:bright
3120:Arabic
2941:Binary
2761:Bubble
2485:Planck
2460:Exotic
2396:Binary
2391:Pulsar
2329:Helium
2290:Barium
2233:Carbon
2226:Yellow
2214:Yellow
2187:Yellow
2026:PG1159
1761:3C 273
1751:NeVe 1
1731:OJ 287
1453:Q star
1319:Issues
1052:Blazar
1042:Quasar
705:
643:
579:
526:
107:energy
40:quasar
3303:Guest
3107:Lists
2988:Super
2642:Fusor
2515:Black
2500:Quark
2480:Preon
2465:Boson
2401:X-ray
2317:Shell
2270:Ap/Bp
2172:Giant
2090:Early
2036:OH/IR
1866:Stars
1494:Lists
995:Micro
965:Rogue
913:Types
802:arXiv
765:arXiv
728:arXiv
703:S2CID
677:arXiv
654:arXiv
641:S2CID
613:arXiv
577:S2CID
551:arXiv
524:S2CID
496:arXiv
488:MNRAS
434:arXiv
331:arXiv
2978:Open
2873:Mass
2697:Core
2647:Nova
2540:Iron
2490:Dark
2300:Lead
2280:HgMn
2275:CEMP
2204:Blue
2177:Blue
2095:Late
1877:List
1463:Geon
1387:Kerr
988:Size
407:2019
381:2019
197:10–2
174:and
149:(2.0
99:mass
91:star
86:and
3279:Sub
3013:Sun
2432:SGR
2209:Red
2182:Red
1057:OVV
1047:LQG
820:doi
798:417
775:doi
761:521
738:doi
724:464
695:doi
673:755
631:doi
609:414
569:doi
547:558
514:doi
492:387
452:doi
430:414
349:doi
327:414
3452::
2312:Be
2265:Am
2248:CH
2243:CN
2162:OB
2157:WR
818:.
810:.
796:.
792:.
773:.
759:.
755:.
736:.
722:.
718:.
701:.
693:.
685:.
671:.
639:.
629:.
621:.
607:.
603:.
575:.
567:.
559:.
545:.
522:.
512:.
504:.
490:.
486:.
466:^
450:.
442:.
428:.
424:.
398:.
372:.
347:.
339:.
325:.
321:.
300:.
286:^
229:.
213:.
182:.
170:,
125:.
70:A
53:.
3368::
2505:Q
2324:B
2238:S
2150:B
2145:O
2133:M
2128:K
2123:G
2118:F
2113:A
2108:B
2103:O
1858:e
1851:t
1844:v
1383:)
1379:(
885:e
878:t
871:v
828:.
822::
814::
804::
783:.
777::
767::
746:.
740::
730::
709:.
697::
689::
679::
662:.
656::
647:.
633::
625::
615::
583:.
571::
563::
553::
530:.
516::
508::
498::
460:.
454::
446::
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409:.
383:.
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351::
343::
333::
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199:Ă—
195:Ă—
151:Ă—
42:.
35:.
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