Recently scientists have used readings of over 1000 Gauss to reinterpret the heating mechanisms of this class of object. The Rossi Explorer captured a superburst of ash on the surface of one in 2004, while a pair of them with a 2.4-hour orbit was discovered by the CSIRO Parkes telescope. Their masses are upper-bounded by the Tolman-Oppenheimer-Volkoff limit. They undergo brief spin-up periods, or glitches, and their accretion of matter from a companion star can result in an equatorial bulge. A hot, rotating one was discovered by Giacconi in Centaurus and their release 
Recently scientists have used readings of over 1000 Gauss to reinterpret the heating mechanisms of this class of object. The Rossi Explorer captured a superburst of ash on the surface of one in 2004, while a pair of them with a 2.4-hour orbit was discovered by the CSIRO Parkes telescope. Their masses are upper-bounded by the Tolman-Oppenheimer-Volkoff limit. They undergo brief spin-up periods, or glitches, and their accretion of matter from a companion star can result in an equatorial bulge. A hot, rotating one was discovered by Giacconi in Centaurus and their release of gravitational binding energy powers supernovae. FTP, name these dense objects first postulated by Baade and Zwicky, whose rotating types are known as pulsars.
Recently scientists have used readings of over 1000 Gauss to reinterpret the heating mechanisms of this class of object.
neutron star