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  • ...], which are bound together by the strong nuclear force, the neutrons in a neutron star are bound together by [[Gravitation|gravity]].
    415 bytes (69 words) - 15:39, 25 January 2023
  • ...upernova, but not so much mass that it forms a [[black hole]] instead of a neutron star.
    192 bytes (33 words) - 15:40, 25 January 2023
  • 12 bytes (1 word) - 15:41, 25 January 2023

Page text matches

  • ...], which are bound together by the strong nuclear force, the neutrons in a neutron star are bound together by [[Gravitation|gravity]].
    415 bytes (69 words) - 15:39, 25 January 2023
  • ...upernova, but not so much mass that it forms a [[black hole]] instead of a neutron star.
    192 bytes (33 words) - 15:40, 25 January 2023
  • ...ut five times the size of the sun, which occurs when the star collapses; a neutron star or a black hole may be formed as a result, or the explosion results in no r
    394 bytes (68 words) - 05:35, 19 July 2010
  • ...ekhar limit]] of 1.4 sun masses. This degenerate object then implodes to a neutron star, but rebound and photodissociation processes also causes the outer parts of ...supernova explosion forming a [[neutron star]].<ref name=StarsCornell/> A neutron star is a very dense body where protons have been converted to neutrons, allowin
    4 KB (664 words) - 16:43, 28 November 2010
  • ...al star discovered to date.<ref>There are smaller planets known around a [[neutron star]], named [[PSR B1257+12]].</ref> The team estimate its radius to be 1.5 tim
    7 KB (1,111 words) - 11:24, 30 July 2022
  • |Neutron Star (final stage)
    15 KB (2,142 words) - 21:59, 7 November 2008
  • ...object]]s: [[brown dwarf]]s, [[black dwarf]]s, cooling [[white dwarf]]s, [[neutron star]]s, and [[black hole]]s. Eventually, as a result of [[relaxation time|gravi
    17 KB (2,688 words) - 22:56, 16 January 2021
  • ...these objects in terms of objects such as [[black hole|black holes]] and [[neutron star|neutron stars]]. [[neutron star|neutron stars]], and [[black hole|black holes]].
    46 KB (6,796 words) - 10:08, 28 February 2024
  • ...e core of a star, or, going even more extreme, inside an atomic nucleus or neutron star. Quick scale for exotic matter: Atomic nuclei and [[Neutron star|neutron stars]] are about 100 trillion times denser than water, which is ab
    45 KB (6,572 words) - 12:36, 9 March 2024
  • Perhaps the highest density known is reached in [[neutron star]] matter (see [[neutronium]]). The [[gravitational singularity|singularity]
    14 KB (2,241 words) - 12:26, 26 October 2021