The March 5 event saw a hard spike of gamma ray radiation from a (*) soft gamma-ray repeater, thought to be this type of star.
An equation named for Lattimer and Swesty is used to model these objects in calculations involving two or more, while the Akmal-Pandharipande-Ravenhall equation of state models their dissipation of energy through the Urca process. These objects contain "swiss cheese" and "spaghetti" phases between their crust and outer cores. The March 5 event saw a hard spike of gamma ray radiation from a (*) soft gamma-ray repeater, thought to be this type of star. These stars occasionally "glitch," but generally spin down through magnetic braking, and their upper mass limit of approximately three solar masses is the Tolman-Oppenheimer-Volkoff limit. For 10 points, pulsars are a type of what stars that are formed when stars between 8 and 20 solar masses undergo a supernova, and are composed entirely of a certain particle?
An equation named for Lattimer and Swesty is used to model these objects in calculations involving two or more, while the Akmal-Pandharipande-Ravenhall equation of state models their dissipation of energy through the Urca process.
{neutron} stars [{accpet} pulsars before mentioned]