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- ...cts are also known under the names '''XDINS''' (X-ray Dim Isolated Neutron Stars) or simply '''XINS'''.<ref name="Potekhin15">{{harvnb|Potekhin|De Luca|Pons ...}}</ref> However, it was soon shown that MS 0317.7-6647 is, in fact, not a neutron star. Then in 2001 a new object fitting this classification was discovered: ...16 KB (2,181 words) - 18:43, 26 December 2024
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- ...Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars|journal = The Astrophysical Journal|volume = 153|pages = 807|year = 1968|la ...e spacetime outside [[neutron stars]], [[white dwarfs]] and [[supermassive stars]]. It can be shown that it is an approximation to the [[Kerr metric]] (whic ...3 KB (386 words) - 19:59, 30 May 2024
- ...e cold phase whose self-gravity is strong enough for them to collapse into stars.{{Citation needed|reason=Because of the claims in this paragraph, each sent ...e can study the dynamics of the cosmic gas and understand the formation of stars. This is just one example. Even magnetohydrodynamics has its basis on the f ...11 KB (1,746 words) - 18:28, 6 August 2024
- ...lessandro |date=2009-10-23 |title=Relativistic tidal properties of neutron stars |url=https://link.aps.org/doi/10.1103/PhysRevD.80.084035 |journal=Physical ...7 KB (991 words) - 19:41, 29 August 2024
- ...cts are also known under the names '''XDINS''' (X-ray Dim Isolated Neutron Stars) or simply '''XINS'''.<ref name="Potekhin15">{{harvnb|Potekhin|De Luca|Pons ...}}</ref> However, it was soon shown that MS 0317.7-6647 is, in fact, not a neutron star. Then in 2001 a new object fitting this classification was discovered: ...16 KB (2,181 words) - 18:43, 26 December 2024
- In 2013, a mass measurement for this [[neutron star]] was announced: slightly over two times the mass of the Sun ({{solar_ ...st2010"/> This measurement confirmed the existence of such massive neutron stars using a different measuring technique. ...12 KB (1,544 words) - 02:29, 30 July 2024
- ...describing the nuclear structure of heavy [[Atomic nucleus|nuclei]] and [[neutron star]]s.<ref>{{cite journal|first1=M. |last1=Baldo |first2=G. F. |last2=Bur ...3 KB (482 words) - 04:59, 17 February 2025
- {{Short description|Binary pulsar–neutron star system}} | class = [[Pulsar]] + [[Neutron star]] ...20 KB (2,633 words) - 17:15, 18 July 2024
- ...ite journal|last=Baiko|first=D A|date=2014-03-25|title=Coulomb crystals in neutron star crust|journal=Journal of Physics: Conference Series|volume=496|pages=0 ...5 KB (668 words) - 07:31, 4 April 2023
- ...0 |title=The Proton-Deuteron Transformation As a Source of Energy in Dense Stars |journal=Physical Review|publisher=American Physical Society |volume=57 |is ...n-rich and free electron-rich environments, such as the inner crust of a [[neutron star]].<ref name=":6" /><ref name=":4">{{Cite journal |last=Zeldovich |firs ...24 KB (3,407 words) - 15:02, 29 October 2024
- ...rong powerful outflows, or winds, of high-energy particles caused by the [[neutron star]]; thus, the sobriquet ''[[black widow (disambiguation)|black widow]]' ...=Kennedy |first14=M. R. |last15=Kramer |first15=M. |date=2023-01-26 |title=Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar bi ...8 KB (1,140 words) - 06:20, 22 December 2023
- {{Short description|Decay of a neutron when outside a nucleus}} The '''inset''' shows beta decay of a free neutron as it is understood today; an electron and antineutrino are created in this ...23 KB (3,067 words) - 16:30, 15 February 2025
- ...are based on excluding known astrophysical alternatives (such as [[neutron stars]]) rather than direct evidence. However, to provide a viable alternative it ...in modified gravity: packing extra effective mass in relativistic compact stars|journal=Physical Review D|volume=92 |issue=6 |pages=064002 |doi=10.1103/10. ...7 KB (934 words) - 07:45, 14 February 2025
- | title = Origin and Evolution of Neutron Star Magnetic Fields ...classical' radio pulsars, 'magnetars', X-ray pulsars), whereas old neutron stars have weak fields ≲ 10<sup>9</sup> [[gauss (unit)|G]] (ms pulsars, lowmass X ...11 KB (1,522 words) - 16:56, 19 January 2025
- {{legend|#9b7bbc|[[neutron emission]]}} ...hich atomic nuclei are unbound with respect to the emission of a proton or neutron. ...33 KB (4,976 words) - 20:45, 23 November 2024
- ...er–Volkoff limit|Tolman–Oppenheimer–Volkoff mass upper limit]] for neutron stars.<ref name="Romani2022"/><ref name="Berkeley"/> The [[pulsar]] rotates at a ...has a mass of {{val|2.35|0.17|u=solar mass}}, making it the most massive [[neutron star]] known {{asof|2022|lc=y}}.<ref name="Romani2022"/> The pulsar likely ...20 KB (2,452 words) - 19:52, 26 December 2024
- ...off |first2=G.M. |author-link2=George Volkoff |year=1939 |title=On Massive Neutron Cores |url=http://www.mpia-hd.mpg.de/home/fendt/Lehre/Vorlesung_CO/1939_opp ...13 KB (1,842 words) - 17:15, 8 January 2025
- ...st massive stars|most massive]] and [[list of most luminous stars|luminous stars known]]. ...was observed in a 2001 survey called the ''Study of Long Period Variables stars near the Galactic Centre''. The survey named the star GMC2001 10-1, GM ...13 KB (1,939 words) - 23:07, 14 August 2024
- | title = Super-dense neutron star is fastest ever seen | url = http://www.space.com/18218-fastest-orbiting-pulsar-neutron-star.html ...10 KB (1,467 words) - 20:42, 21 January 2024
- ...<math> R_S </math>, suggesting that only [[Black Hole|black holes]] and [[neutron star]]s have innermost stable circular orbits outside of their surfaces. As {{Portal bar|Physics|Mathematics|Astronomy|Stars|Spaceflight|Outer space|Science}} ...8 KB (1,266 words) - 15:24, 17 November 2024
- ...}}</ref><ref name="a+2016">{{cite journal |title=Properties of the binary neutron star merger GW170817 |first1=B. P. |last1=Abbott |journal=Physical Review X |title=Source Redshifts from Gravitational-Wave Observations of Binary Neutron Star Mergers ...10 KB (1,479 words) - 17:58, 18 July 2024