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The 69 pages that link to Neutron star, each with the reason it gives.

• X-ray astronomyRelated: Its surface, magnetic field, and accretion flows can produce distinctive X-ray signals.

• SupernovaRelated: Core collapse can leave this compact object at the center of the ejecta.

• Supernova remnantRelated: A neutron star can remain near the center of a core-collapse remnant.

• Core-collapse supernovaRelated: It is a common compact remnant left by core collapse.

• Relativistic jetRelated: Some accreting neutron stars also produce relativistic jets, linking the phenomenon to more than black holes.

• Stellar massRelated: The remnant mass after a supernova can leave a neutron star.

• Gravitational binding energyRelated: Its extreme compactness gives it exceptionally large gravitational binding energy per unit mass.

• SN 1987ARelated: Whether SN 1987A left a neutron star was long uncertain; evidence for a compact remnant has since emerged.

• Nuclear drip lineRelated: Drip-line physics informs models of matter at densities approaching those inside neutron stars.

• Fermi gasRelated: Neutron matter provides a high-density setting for Fermi-gas reasoning.

• Fritz ZwickyRelated: Zwicky proposed that supernova explosions could produce neutron stars.

• Red supergiantRelated: It is one possible compact remnant of a red supergiant's collapse.

• Subrahmanyan ChandrasekharRelated: His work helped establish that stars beyond the white-dwarf limit require different final states.

• Walter BaadeRelated: Baade and Zwicky proposed neutron stars as possible products of supernovae.

• Quantum degeneracyRelated: Neutron degeneracy contributes to its support, alongside nuclear interactions.

• Up quarkRelated: Its matter is built from nucleons containing up quarks, with deeper phases still investigated.

• Color superconductivityRelated: Its core may reach densities at which deconfined quark matter and pairing are possible.

• HyperonRelated: Hyperons may appear at high densities and alter the star's predicted structure.

• Bondi accretionRelated: Its gravity can capture surrounding gas, while its surface and magnetic field add physics absent from the basic model.

• HypernucleusRelated: Hypernuclear interactions help assess whether hyperons can exist in neutron-star interiors.

• Type II supernovaRelated: A successful collapse explosion commonly leaves a neutron star at its center.

• QCD matterRelated: Its core may contain dense phases of QCD matter not yet confirmed.