3386:
991:
57:
3446:
3348:
1821:
69:
3410:
3434:
1831:
3398:
3422:
3359:
231:
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
204:, 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
172:
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
552:
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".
152:, 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
3199:
1453:
227:
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
1117:
1217:
1391:
308:
3385:
3231:
894:
852:
3206:
2525:
1433:
1522:
678:
Czerny, Bozena; Janiuk, Agnieszka; Sikora, Marek; Lasota, Jean-Pierre (2012). "Quasi-Star Jets as
Unidentified Gamma-Ray Sources".
1402:
1517:
380:
2918:
1438:
1234:
2832:
980:
3211:
2848:
1867:
1660:
1341:
3258:
3125:
1428:
1303:
1249:
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3182:
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1615:
1605:
190:
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3246:
3177:
3147:
1336:
1288:
1271:
970:
280:
3253:
3130:
3107:
2689:
2138:
2133:
2128:
2123:
2118:
2113:
1791:
1293:
1207:
955:
887:
2396:
2270:
1905:
1468:
727:"Light or heavy supermassive black hole seeds: The role of internal rotation in the fate of supermassive stars"
250:
2923:
2592:
1716:
3172:
2722:
2632:
2574:
2500:
2071:
1997:
1645:
1181:
1144:
1047:
1042:
960:
406:
233:
217:
133:
124:
at its core. They were first proposed in the 1960s and have since provided valuable insights into the early
105:
1947:
1834:
1407:
3333:
3313:
3085:
3080:
2873:
2822:
2627:
2617:
2290:
2088:
2056:
1930:
1675:
1563:
1548:
1100:
990:
914:
3187:
3157:
3152:
3142:
3070:
2858:
2024:
1553:
1366:
1110:
965:
61:
2305:
1283:
196:
Once the black hole had formed at the protostar's core, it would continue generating a large amount of
3466:
3328:
3226:
3216:
3065:
3033:
2827:
2622:
2607:
1920:
1824:
1532:
1504:
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1315:
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935:
880:
822:
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633:
571:
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454:
351:
2167:
200:
from the infall of stellar material. This constant outburst of energy would counteract the force of
3471:
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2771:
2442:
2344:
1655:
1630:
1600:
1558:
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384:
236:
at or below this limiting temperature. The object would then quickly dissipate, leaving behind the
3426:
3414:
3323:
3284:
3236:
3221:
3135:
3075:
2998:
2908:
2878:
2868:
2812:
2734:
2425:
2061:
1860:
1489:
1361:
1266:
1072:
1057:
1025:
950:
945:
812:
775:
738:
713:
687:
664:
651:
623:
587:
561:
534:
506:
444:
341:
253: – Accumulation of particles into a massive object by gravitationally attracting more matter
31:
1077:
3274:
2759:
2699:
2672:
2652:
2452:
2236:
2224:
2051:
2031:
1985:
1967:
1935:
1635:
1625:
1620:
1356:
1320:
1308:
1261:
1202:
1171:
1161:
1095:
169:
90:
1796:
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3102:
3055:
3005:
2993:
2971:
2966:
2893:
2853:
2800:
2582:
2505:
2480:
2374:
2295:
2019:
1980:
1786:
1746:
1494:
1443:
1298:
1212:
1005:
975:
830:
785:
748:
705:
641:
579:
575:
524:
462:
359:
259: – Structure formed by diffuse material in orbital motion around a massive central body
178:
165:
56:
132:. Although they have not been observed, they are considered to be a possible progenitor of
3289:
3092:
2961:
2805:
2776:
2717:
2712:
2587:
2315:
2280:
2214:
2160:
2155:
2100:
1910:
1806:
1756:
1731:
1527:
1371:
1278:
1244:
1156:
431:
Ball, Warrick H.; Tout, Christopher A.; Żytkow, Anna N.; Eldridge, John J. (1 July 2011).
221:
1706:
826:
701:
637:
520:
458:
433:"The structure and evolution of quasi-stars: The structure and evolution of quasi-stars"
355:
3450:
3390:
3351:
3117:
2956:
2783:
2754:
2729:
2662:
2351:
2219:
2105:
2007:
1897:
1887:
1721:
1473:
1412:
1256:
930:
256:
197:
174:
113:
43:
709:
3460:
3303:
3097:
3060:
3028:
2903:
2612:
2435:
2406:
2384:
2002:
1975:
1952:
1853:
1781:
1701:
1229:
1224:
835:
800:
717:
655:
646:
611:
591:
529:
494:
467:
432:
410:
364:
329:
313:
538:
3445:
3363:
3038:
2988:
2983:
2883:
2766:
2749:
2707:
2667:
2602:
2485:
2430:
2411:
2391:
2369:
2361:
2204:
2197:
2036:
1957:
1940:
1736:
1610:
1578:
1186:
1105:
610:
Ball, Warrick H.; Tout, Christopher A.; Żytkow, Anna N.; Eldridge, John J. (2011).
328:
Ball, Warrick H.; Tout, Christopher A.; Żytkow, Anna N.; Eldridge, John J. (2011).
274:
68:
583:
1776:
3279:
2978:
2951:
2943:
2933:
2913:
2888:
2817:
2739:
2495:
2470:
2465:
2379:
2339:
2300:
2265:
2248:
2243:
1915:
1726:
1680:
1583:
1458:
1397:
1122:
1030:
129:
108:. They are thought to have lived around 7-10 million years due to their immense
39:
2863:
2560:
2510:
2490:
2475:
2327:
2231:
2209:
2187:
2182:
2046:
1766:
1696:
1665:
1593:
1588:
1573:
1239:
1166:
1067:
903:
864:
860:
663:
Ball, Warrick H. (2012). "Quasi-stars and the Schönberg-Chandrasekhar limit".
228:
157:
149:
121:
98:
3050:
2898:
2682:
2647:
2642:
2637:
2597:
2550:
2540:
2334:
2310:
2285:
2192:
2143:
2076:
2066:
2041:
2014:
1990:
1925:
1801:
1448:
1351:
1139:
1134:
790:
763:
753:
726:
186:
182:
153:
145:
35:
764:"Modelling supermassive primordial stars with <SCP>mesa</SCP>"
30:"Black hole star" redirects here. For black holes created from stars, see
3043:
2744:
2418:
2177:
2150:
1711:
1670:
1568:
125:
73:
17:
3318:
2793:
2555:
2322:
2275:
2258:
2253:
2172:
1751:
262:
201:
853:"Quasi-Stars: Black Holes at the Core of the Universe's Largest Stars"
3308:
3296:
2515:
2401:
1771:
1761:
1741:
1463:
1062:
1052:
762:
Herrington, Nicholas P.; Whalen, Daniel J.; Woods, Tyrone E. (2023).
117:
50:
3358:
780:
743:
817:
692:
669:
628:
566:
511:
449:
346:
168:
drawing in enormous amounts of gas via gravity, which can produce
67:
55:
801:"A lower limit on the halo mass to form supermassive black holes"
2677:
2657:
1876:
109:
101:
94:
1849:
876:
3023:
872:
495:"Quasi-stars: accreting black holes inside massive envelopes"
60:
Size comparison of a hypothetical quasi-star to some of the
407:"Cooking up supermassive black holes in the early universe"
144:
A quasi-star would have resulted from the core of a large
1845:
799:
Dotan, Calanit; Rossi, Elena M.; Shaviv, Nir J. (2011).
493:
Begelman, Mitch; Rossi, Elena; Armitage, Philip (2008).
27:
Hypothetical early-universe star with a black hole core
3374:
38:. For types of stars denser than neutron stars, see
3267:
3116:
3014:
2942:
2841:
2698:
2573:
2451:
2360:
2087:
1966:
1896:
1689:
1541:
1503:
1482:
1421:
1380:
1329:
1195:
1088:
998:
923:
381:"Zeroing In on How Supermassive Black Holes Formed"
164:10 kg). Quasi-stars may have also formed from
309:"Biggest black holes may grow inside 'quasistars'"
49:Not to be confused with a quasi-stellar object or
805:Monthly Notices of the Royal Astronomical Society
768:Monthly Notices of the Royal Astronomical Society
731:Monthly Notices of the Royal Astronomical Society
616:Monthly Notices of the Royal Astronomical Society
437:Monthly Notices of the Royal Astronomical Society
334:Monthly Notices of the Royal Astronomical Society
216:have been suggested as the progenitors of modern
866:Black Hole Star – The Star That Shouldn't Exist
156:. Such a star would have to be at least 1,000
1861:
888:
8:
612:"The structure and evolution of quasi-stars"
330:"The structure and evolution of quasi-stars"
112:. Unlike modern stars, which are powered by
2093:
1868:
1854:
1846:
1454:Magnetospheric eternally collapsing object
895:
881:
873:
725:Fiacconi, Davide; Rossi, Elena M. (2017).
834:
816:
789:
779:
752:
742:
691:
668:
645:
627:
565:
528:
510:
466:
448:
379:Saplakoglu, Yasemin (29 September 2017).
363:
345:
265: – Hypothetical type of neutron star
34:. For stars that become black holes, see
302:
300:
298:
277: – Collapsed core of a massive star
128:, galaxy formation, and the behavior of
120:would come from material falling into a
3381:
488:
486:
484:
482:
480:
478:
307:Battersby, Stephen (29 November 2007).
294:
405:Johnson-Goh, Mara (20 November 2017).
271: – Hypothetical hybrid star type
42:. For the 1994 Soundgarden song, see
7:
1830:
222:the one in the center of the Galaxy
104:that may have existed early in the
283: – High-mass black hole seeds
25:
3444:
3432:
3420:
3408:
3396:
3384:
3357:
3347:
3346:
1829:
1820:
1819:
1118:Tolman–Oppenheimer–Volkoff limit
989:
836:10.1111/j.1365-2966.2011.19461.x
647:10.1111/j.1365-2966.2011.18591.x
530:10.1111/j.1365-2966.2008.13344.x
468:10.1111/j.1365-2966.2011.18591.x
365:10.1111/j.1365-2966.2011.18591.x
1235:Innermost stable circular orbit
116:in their cores, a quasi-star's
1661:Timeline of black hole physics
177:stars. Such stars would dwarf
1:
3259:Timeline of stellar astronomy
1429:Nonsingular black hole models
214:intermediate-mass black holes
554:Astronomy & Astrophysics
238:intermediate mass black hole
2919:Hertzsprung–Russell diagram
1651:Rossi X-ray Timing Explorer
1616:Hypercompact stellar system
1606:Gamma-ray burst progenitors
710:10.1088/2041-8205/755/1/L15
584:10.1051/0004-6361/201321949
72:A quasi-star rendered with
3493:
2833:Kelvin–Helmholtz mechanism
1337:Black hole complementarity
1304:Bousso's holographic bound
1289:Quasi-periodic oscillation
987:
981:Malament–Hogarth spacetime
281:Direct collapse black hole
191:largest known modern stars
48:
29:
3342:
2096:
1883:
1815:
1208:Gravitational singularity
910:
680:The Astrophysical Journal
3212:With multiple exoplanets
1792:PSO J030947.49+271757.31
1717:SDSS J150243.09+111557.3
1250:Blandford–Znajek process
251:Accretion (astrophysics)
218:supermassive black holes
140:Formation and properties
134:supermassive black holes
1998:Asymptotic giant branch
1048:Active galactic nucleus
576:2013A&A...558A..59S
234:hydrostatic equilibrium
106:history of the Universe
3334:Tidal disruption event
2823:Circumstellar envelope
2057:Luminous blue variable
1676:Tidal disruption event
1646:Supermassive dark star
1564:Black holes in fiction
1549:Outline of black holes
1182:Supermassive dark star
1101:Gravitational collapse
76:
65:
2859:Effective temperature
1554:Black Hole Initiative
1367:Holographic principle
791:10.1093/mnras/stad572
754:10.1093/mnras/stw2505
71:
59:
3329:Planet-hosting stars
3207:With resolved images
3178:Historical brightest
3108:Photometric-standard
3034:Solar radio emission
2828:Eddington luminosity
2608:Triple-alpha process
2546:Thorne–Żytkow object
1921:Young stellar object
1357:Final parsec problem
1316:Schwarzschild radius
863:(15 December 2022),
269:Thorne–Żytkow object
3153:Highest temperature
2924:Color–color diagram
2789:Protoplanetary disk
2593:Proton–proton chain
2271:Chemically peculiar
1656:Superluminal motion
1631:Population III star
1601:Gravitational waves
1559:Black hole starship
1342:Information paradox
827:2011MNRAS.417.3035D
702:2012ApJ...755L..15C
638:2011MNRAS.414.2751B
521:2008MNRAS.387.1649B
459:2011MNRAS.414.2751B
385:Scientific American
356:2011MNRAS.414.2751B
212:10 kg). These
62:largest known stars
3477:Hypothetical stars
3158:Lowest temperature
2909:Photometric system
2879:Absolute magnitude
2813:Circumstellar dust
2426:Stellar black hole
2062:Stellar population
1948:Herbig–Haro object
1490:Optical black hole
1403:Reissner–Nordström
1362:Firewall (physics)
1267:Gravitational lens
189:, three among the
170:supermassive stars
148:collapsing into a
77:
66:
32:Stellar black hole
3372:
3371:
3275:Substellar object
3254:Planetary nebulae
2673:Luminous red nova
2583:Deuterium burning
2569:
2568:
2052:Instability strip
2032:Wolf-Rayet nebula
1986:Horizontal branch
1931:Pre-main-sequence
1843:
1842:
1636:Supermassive star
1626:Naked singularity
1621:Membrane paradigm
1347:Cosmic censorship
1321:Spaghettification
1309:Immirzi parameter
1262:Hawking radiation
1203:Astrophysical jet
1172:Supermassive star
1162:Binary black hole
1096:Stellar evolution
1038:Intermediate-mass
166:dark matter halos
91:hypothetical type
16:(Redirected from
3484:
3449:
3448:
3437:
3436:
3435:
3425:
3424:
3423:
3413:
3412:
3411:
3401:
3400:
3399:
3389:
3388:
3380:
3364:Stars portal
3362:
3361:
3350:
3349:
3006:Planetary system
2929:Strömgren sphere
2801:Asteroseismology
2522:Black hole star
2094:
2020:Planetary nebula
1981:Red-giant branch
1870:
1863:
1856:
1847:
1833:
1832:
1823:
1822:
1495:Sonic black hole
1444:Dark-energy star
1299:Bekenstein bound
1284:M–sigma relation
1213:Ring singularity
993:
897:
890:
883:
874:
869:
856:
840:
838:
820:
811:(4): 3035–3046.
795:
793:
783:
758:
756:
746:
737:(2): 2259–2269.
721:
695:
674:
672:
659:
649:
631:
622:(3): 2751–2762.
596:
595:
569:
549:
543:
542:
532:
514:
505:(4): 1649–1659.
490:
473:
472:
470:
452:
443:(3): 2751–2762.
428:
422:
421:
419:
417:
402:
396:
395:
393:
391:
376:
370:
369:
367:
349:
340:(3): 2751–2762.
325:
319:
318:
304:
211:
207:
179:VY Canis Majoris
163:
21:
3492:
3491:
3487:
3486:
3485:
3483:
3482:
3481:
3457:
3456:
3455:
3443:
3433:
3431:
3421:
3419:
3409:
3407:
3397:
3395:
3383:
3375:
3373:
3368:
3356:
3338:
3263:
3232:Milky Way novae
3168:Smallest volume
3112:
3093:Radial velocity
3016:
3010:
2962:Common envelope
2938:
2837:
2806:Helioseismology
2777:Bipolar outflow
2718:Microturbulence
2713:Convection zone
2694:
2588:Lithium burning
2575:Nucleosynthesis
2565:
2447:
2356:
2083:
1962:
1911:Molecular cloud
1892:
1879:
1874:
1844:
1839:
1811:
1787:ULAS J1342+0928
1747:SDSS J0849+1114
1732:Phoenix Cluster
1685:
1537:
1499:
1478:
1417:
1376:
1372:No-hair theorem
1325:
1279:Bondi accretion
1245:Penrose process
1191:
1157:Gamma-ray burst
1084:
994:
985:
971:Direct collapse
919:
906:
901:
859:
851:
848:
843:
798:
761:
724:
677:
662:
609:
605:
603:Further reading
600:
599:
551:
550:
546:
492:
491:
476:
430:
429:
425:
415:
413:
404:
403:
399:
389:
387:
378:
377:
373:
327:
326:
322:
306:
305:
296:
291:
286:
246:
209:
205:
161:
142:
87:black hole star
54:
47:
28:
23:
22:
15:
12:
11:
5:
3490:
3488:
3480:
3479:
3474:
3469:
3459:
3458:
3454:
3453:
3441:
3429:
3417:
3405:
3393:
3370:
3369:
3367:
3366:
3354:
3343:
3340:
3339:
3337:
3336:
3331:
3326:
3321:
3316:
3311:
3306:
3301:
3300:
3299:
3294:
3293:
3292:
3287:
3271:
3269:
3265:
3264:
3262:
3261:
3256:
3251:
3250:
3249:
3244:
3234:
3229:
3224:
3219:
3214:
3209:
3204:
3203:
3202:
3197:
3196:
3195:
3185:
3180:
3175:
3170:
3165:
3163:Largest volume
3160:
3155:
3150:
3140:
3139:
3138:
3133:
3122:
3120:
3114:
3113:
3111:
3110:
3105:
3100:
3095:
3090:
3089:
3088:
3083:
3078:
3068:
3063:
3058:
3053:
3048:
3047:
3046:
3041:
3036:
3031:
3020:
3018:
3012:
3011:
3009:
3008:
3003:
3002:
3001:
2996:
2991:
2981:
2976:
2975:
2974:
2969:
2964:
2959:
2948:
2946:
2940:
2939:
2937:
2936:
2931:
2926:
2921:
2916:
2911:
2906:
2901:
2896:
2891:
2886:
2881:
2876:
2874:Magnetic field
2871:
2866:
2861:
2856:
2851:
2845:
2843:
2839:
2838:
2836:
2835:
2830:
2825:
2820:
2815:
2810:
2809:
2808:
2798:
2797:
2796:
2791:
2784:Accretion disk
2781:
2780:
2779:
2774:
2764:
2763:
2762:
2760:Alfvén surface
2757:
2755:Stellar corona
2752:
2747:
2742:
2732:
2730:Radiation zone
2727:
2726:
2725:
2720:
2710:
2704:
2702:
2696:
2695:
2693:
2692:
2687:
2686:
2685:
2680:
2675:
2670:
2665:
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2110:Main sequence
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2089:Classification
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2017:
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1807:Swift J1644+57
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1757:MS 0735.6+7421
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1722:Sagittarius A*
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1294:Thermodynamics
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1257:Accretion disk
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931:BTZ black hole
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855:. 16 May 2020.
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1150:Related links
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70:
63:
58:
52:
45:
41:
37:
33:
19:
3439:Solar System
3227:White dwarfs
3217:Brown dwarfs
3200:Most distant
3148:Most massive
3126:Proper names
3086:Photographic
3039:Solar System
3017:observations
2944:Star systems
2767:Stellar wind
2750:Chromosphere
2723:Oscillations
2603:Helium flash
2533:
2453:Hypothetical
2431:X-ray binary
2370:Compact star
2205:Bright giant
1958:Henyey track
1936:Herbig Ae/Be
1737:PKS 1302-102
1640:
1611:Gravity well
1579:Compact star
1533:Microquasars
1518:Most massive
1422:Alternatives
1187:X-ray binary
1176:
1106:Neutron star
1043:Supermassive
1020:Hawking star
961:Supermassive
865:
808:
804:
771:
767:
734:
730:
683:
679:
619:
615:
557:
553:
547:
502:
498:
440:
436:
426:
414:. Retrieved
400:
388:. Retrieved
374:
337:
333:
323:
312:
275:Neutron star
226:
195:
158:solar masses
143:
86:
82:
80:
78:
3467:Black holes
3427:Outer space
3415:Spaceflight
3280:Brown dwarf
3056:Circumpolar
2934:Kraft break
2914:Color index
2889:Metallicity
2849:Designation
2818:Cosmic dust
2740:Photosphere
2506:Dark-energy
2481:Electroweak
2466:Black dwarf
2397:Radio-quiet
2380:White dwarf
2266:White dwarf
1916:Bok globule
1727:Centaurus A
1681:Planet Nine
1584:Exotic star
1513:Black holes
1459:Planck star
1408:Kerr–Newman
1123:White dwarf
1073:Radio-Quiet
1031:Microquasar
904:Black holes
774:: 463–473.
187:VV Cephei A
130:black holes
40:Exotic star
3472:Star types
3461:Categories
3242:Candidates
3237:Supernovae
3222:Red dwarfs
3081:Extinction
2869:Kinematics
2864:Luminosity
2842:Properties
2735:Atmosphere
2633:Si burning
2623:Ne burning
2561:White hole
2534:Quasi-star
2461:Blue dwarf
2316:Technetium
2232:Hypergiant
2210:Supergiant
1777:Q0906+6930
1767:Hercules A
1697:Cygnus X-1
1666:White hole
1641:Quasi-star
1594:Preon star
1589:Quark star
1574:Big Bounce
1434:Black star
1392:Derivation
1240:Ergosphere
1196:Properties
1177:Quasi-star
1167:Quark star
1078:Radio-Loud
966:Primordial
956:Kugelblitz
861:Kurzgesagt
781:2208.00008
744:1604.03936
686:(1): L15.
289:References
154:supernovae
150:black hole
122:black hole
83:quasi-star
3403:Astronomy
3173:Brightest
3071:Magnitude
3051:Pole star
2972:Symbiotic
2967:Eclipsing
2899:Starlight
2700:Structure
2690:Supernova
2683:Micronova
2678:Recurrent
2663:Symbiotic
2648:p-process
2643:r-process
2638:s-process
2628:O burning
2618:C burning
2598:CNO cycle
2541:Gravastar
2077:Hypernova
2067:Supernova
2042:Dredge-up
2015:Blue loop
2008:super-AGB
1991:Red clump
1968:Evolution
1926:Protostar
1906:Accretion
1898:Formation
1802:AT2018hyz
1449:Gravastar
1439:Dark star
1272:Microlens
1145:Hypernova
1140:Micronova
1135:Supernova
1089:Formation
818:1107.3562
718:113397287
693:1207.1560
670:1207.5972
656:119239346
629:1102.5098
592:119197147
567:1305.5923
512:0711.4078
450:1102.5098
347:1102.5098
183:Mu Cephei
146:protostar
36:Supernova
18:Quasistar
3352:Category
3247:Remnants
3143:Extremes
3103:Parallax
3076:Apparent
3066:Asterism
3044:Sunlight
2994:Globular
2979:Multiple
2904:Variable
2894:Rotation
2854:Dynamics
2745:Starspot
2419:Magnetar
2362:Remnants
2178:Subgiant
2151:Subdwarf
2003:post-AGB
1825:Category
1712:A0620-00
1671:Wormhole
1569:Big Bang
1469:Fuzzball
1352:ER = EPR
1218:Theorems
1016:Electron
1011:Extremal
941:Rotating
539:12044015
244:See also
229:luminous
220:such as
126:universe
99:luminous
74:Celestia
3451:Science
3391:Physics
3377:Portals
3319:Gravity
3268:Related
3188:Nearest
3136:Chinese
2984:Cluster
2957:Contact
2794:Proplyd
2668:Remnant
2556:Blitzar
2530:Hawking
2486:Strange
2436:Burster
2392:Neutron
2345:Extreme
2296:He-weak
1941:T Tauri
1835:Commons
1797:P172+18
1752:TON 618
1690:Notable
1542:Related
1528:Quasars
1523:Nearest
1483:Analogs
1413:Hayward
1381:Metrics
1026:Stellar
951:Virtual
946:Charged
915:Outline
823:Bibcode
698:Bibcode
634:Bibcode
572:Bibcode
560:: A59.
517:Bibcode
455:Bibcode
416:8 April
390:8 April
352:Bibcode
263:Blitzar
202:gravity
95:massive
89:) is a
3309:Galaxy
3297:Planet
3285:Desert
3193:bright
3131:Arabic
2952:Binary
2772:Bubble
2496:Planck
2471:Exotic
2407:Binary
2402:Pulsar
2340:Helium
2301:Barium
2244:Carbon
2237:Yellow
2225:Yellow
2198:Yellow
2037:PG1159
1772:3C 273
1762:NeVe 1
1742:OJ 287
1464:Q star
1330:Issues
1063:Blazar
1053:Quasar
716:
654:
590:
537:
118:energy
51:quasar
3314:Guest
3118:Lists
2999:Super
2653:Fusor
2526:Black
2511:Quark
2491:Preon
2476:Boson
2412:X-ray
2328:Shell
2281:Ap/Bp
2183:Giant
2101:Early
2047:OH/IR
1877:Stars
1505:Lists
1006:Micro
976:Rogue
924:Types
813:arXiv
776:arXiv
739:arXiv
714:S2CID
688:arXiv
665:arXiv
652:S2CID
624:arXiv
588:S2CID
562:arXiv
535:S2CID
507:arXiv
499:MNRAS
445:arXiv
342:arXiv
2989:Open
2884:Mass
2708:Core
2658:Nova
2551:Iron
2501:Dark
2311:Lead
2291:HgMn
2286:CEMP
2215:Blue
2188:Blue
2106:Late
1888:List
1474:Geon
1398:Kerr
999:Size
418:2019
392:2019
208:10–2
185:and
160:(2.0
110:mass
102:star
97:and
3290:Sub
3024:Sun
2443:SGR
2220:Red
2193:Red
1068:OVV
1058:LQG
831:doi
809:417
786:doi
772:521
749:doi
735:464
706:doi
684:755
642:doi
620:414
580:doi
558:558
525:doi
503:387
463:doi
441:414
360:doi
338:414
3463::
2323:Be
2276:Am
2259:CH
2254:CN
2173:OB
2168:WR
829:.
821:.
807:.
803:.
784:.
770:.
766:.
747:.
733:.
729:.
712:.
704:.
696:.
682:.
650:.
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632:.
618:.
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586:.
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570:.
556:.
533:.
523:.
515:.
501:.
497:.
477:^
461:.
453:.
439:.
435:.
409:.
383:.
358:.
350:.
336:.
332:.
311:.
297:^
240:.
224:.
193:.
181:,
136:.
81:A
64:.
3379::
2516:Q
2335:B
2249:S
2161:B
2156:O
2144:M
2139:K
2134:G
2129:F
2124:A
2119:B
2114:O
1869:e
1862:t
1855:v
1394:)
1390:(
896:e
889:t
882:v
839:.
833::
825::
815::
794:.
788::
778::
757:.
751::
741::
720:.
708::
700::
690::
673:.
667::
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210:Ă—
206:Ă—
162:Ă—
53:.
46:.
20:)
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