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88:. This instability is believed to limit the mass of main-sequence stars to a couple of hundred solar masses or so. Stars of this size and larger are able to directly collapse into a black hole of either
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is the most rapidly rotating star ever found - ~ 200 times faster than the sun, or with a speed of 447 kilometres per second (1,610,000 km/h)
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54:. Rotating supermassive stars are a hypothetical form of a relativistic star. Relativistic stars are one possible source to allow
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84:. Stability analysis shows that such a star is only marginally bound, and is unstable to either collapse or
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Numerical
Relativity: Solving Einstein's Equations on the Computer
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Baumgarte, Thomas W.; Shapiro, Stuart L. (June 24, 2010).
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Another definition of a relativistic star is one with the
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Timeline of white dwarfs, neutron stars, and supernovae
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139:"Fastest Rotating Star Found in Neighboring Galaxy"
69:gas. This can happen when the core of a massive
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46:. The first such object to be identified was
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164:. Cambridge University Press. p. 459.
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729:This article about stellar astronomy is a
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204:Relativistic stars, recommended reading
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209:Pair instability chart (Archived copy)
7:
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73:star becomes hot enough to generate
38:whose behavior is well described by
185:Nikolaos Stergioulas (2003-03-07).
733:. You can help Knowledge (XXG) by
14:
114:"VLT Finds Fastest Rotating Star"
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697:
688:
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451:Tolman–Oppenheimer–Volkoff limit
634:Fermi Gamma-ray Space Telescope
187:"Rotating Stars in Relativity"
1:
660:X-ray pulsar-based navigation
639:Compton Gamma Ray Observatory
50:, which consist of rotating
629:Rossi X-ray Timing Explorer
472:Gamma-ray burst progenitors
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716:
426:Quasi-periodic oscillation
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644:Chandra X-ray Observatory
411:Neutron-star oscillation
300:Rotating radio transient
790:Stellar astronomy stubs
665:Tempo software program
27:
675:The Magnificent Seven
22:
780:Theory of relativity
580:Thorne–Żytkow object
67:special relativistic
531:Neutron star merger
391:Chandrasekhar limit
358:Hulse–Taylor pulsar
285:Soft gamma repeater
118:ESO Science Release
56:gravitational waves
44:classical mechanics
575:Pulsar wind nebula
553:Stellar black hole
40:general relativity
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504:Supernova remnant
294:Ultra-long period
63:equation of state
32:relativistic star
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477:Asteroseismology
379:Fast radio burst
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16:Category of star
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58:to be studied.
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273:Single pulsars
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198:External links
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34:is a rotating
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622:investigation
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570:Pulsar planet
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558:Related links
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546:Related links
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509:Related links
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331:X-ray burster
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71:main-sequence
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52:neutron stars
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48:radio pulsars
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42:, but not by
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25:
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735:expanding it
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482:Compact star
456:Urca process
446:Timing noise
431:Relativistic
430:
326:X-ray binary
321:X-ray pulsar
245:Neutron star
180:
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142:. Retrieved
133:
121:. Retrieved
117:
108:
94:supermassive
90:intermediate
60:
31:
29:
541:White dwarf
526:Microquasar
492:Exotic star
421:Pulsar kick
343:Millisecond
259:Radio-quiet
123:12 December
785:Star types
774:Categories
670:Astropulse
585:QCD matter
565:Radio star
536:Quark-nova
487:Quark star
436:Rp-process
367:Properties
144:2011-12-29
100:References
620:Satellite
594:Discovery
516:Hypernova
499:Supernova
441:Starquake
693:Category
521:Kilonova
348:Be/X-ray
280:Magnetar
79:positron
75:electron
24:VFTS 102
703:Commons
465:Related
416:Optical
374:Blitzar
353:Spin-up
86:explode
401:Glitch
316:Binary
264:Pulsar
168:
96:size.
653:Other
601:LGM-1
252:Types
82:pairs
65:of a
731:stub
336:List
166:ISBN
125:2011
36:star
92:or
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116:.
30:A
762:e
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748:v
737:.
237:e
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174:.
147:.
127:.
77:-
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
