These stars have an upper limit of about 3 solar masses, which is higher than the Chandresekhar limit for white dwarf stars.
The outer regions of these objects may be subject to non-dissipative entrainment of coupled superfluids according to multifluid models. These stars experience a namesake kick by which they move much faster than their progenitor stars. One of these objects at the center of the Crab Nebula is thought to be the reason for its continued visibility. Jocelyn Bell discovered a type of these stars but instead her advisor Anthony Hewish got the Nobel Prize. One important binary system of two of these will inspiral in about three hundred million years because it's losing energy to gravitational radiation. That system is named for Hulse and Taylor. These stars have an upper limit of about 3 solar masses, which is higher than the Chandresekhar limit for white dwarf stars. For 10 points, name these stars which are supported from collapse by degeneracy pressure of their namesake neutral particles.
The outer regions of these objects may be subject to non-dissipative entrainment of coupled superfluids according to multifluid models.
neutron stars (accept pulsars)