KnowraNeutron starLinked fromLinked fromThe 69 pages that link to Neutron star, each with the reason it gives.All 69Broader topic 17Related 22Narrower topic 19Compared with 11White dwarfCompared with: It is generally denser than a white dwarf and forms from more massive stellar progenitors.Black holeCompared with: Unlike a black hole, it has a material surface outside its compact interior.Electron degeneracy pressureCompared with: Its support involves neutron degeneracy and nuclear interactions rather than electron degeneracy alone.Chandrasekhar limitCompared with: Collapse beyond white-dwarf support can lead toward a neutron-star remnant.Primordial black holeCompared with: Neutron stars can mimic some compact-lens signals without being black holes.Cygnus X-1Compared with: Neutron stars can also power X-ray binaries, but have surfaces and distinct emission signatures.Quark starCompared with: It is the standard comparison: quark stars would contain deconfined matter at greater density.Stellar black holeCompared with: A neutron star is the alternative remnant when collapse stops short of forming a black hole.Astronomical black holesCompared with: It is the main alternative compact remnant when a collapsing stellar core avoids becoming a black hole.Black dwarfCompared with: More massive stellar cores can become neutron stars rather than white dwarfs.Micro black holeCompared with: A neutron star can be tiny by astronomical standards without being a microscopic black hole.