... that although are small in size (I.e in radius), they more than make up for it in mass; neutron stars. Neutron stars are the smallest, densest known stars to exist and they typically have a radius of around 10 kilometres (6.2 miles), but have masses...
... Earth-bound chroniclers as early as 1054 A.D. The remaining compact and very dense neutron star, is so-called because the star’s main constituent is neutrons, produced when the collapsing core essentially melts protons and electrons into each other...
... from the first black hole-neutron star merger and the first binary neutron star merger; an event which also... starting to appreciate the wonderful diversity of black holes and neutron stars. Our latest results prove that they come in many sizes...
... has approved funding to the MEESST (Magnetohydrodynamic Enhanced Entry System for Space Transportation) consortium, of which both Neutron Star Systems and the University of Stuttgart (IRS) are members. The project will design, build, and test...
... millisecond pulsar, PSR 1937+21, was also discovered in 1982. It has a pulse period of 1.6 milliseconds, meaning that the neutron star is rotating 640 times each second. This established the existence of a second class of pulsars and required new...
... can be grouped into two categories: FRBs are either caused by relatively rare explosive collisions between old neutron stars or white dwarfs, or they are more common, periodic outbursts or flares from younger, rapidly spinning pulsars. The...