Black holes, white dwarfs, and neutron stars Saul A. Teukolsky, Stuart L. Shapiro
Publisher: John Wiley & Sons Inc

If a star is much greater than 3 times our Sun's mass it will form a black hole at its death. In many binary star systems, the primary star is a compact object such as a black hole, a neutron star, or white dwarf. RXTE sent data from its last science observation to the ground early on Jan. Our Sun is expected to end as a white dwarf after it is a red giant. They suggest that two compact stellar remnants, i.e. Neutron star simulation in Astrophysics is being discussed at Physics Forums. Black holes, like neutron stars, white dwarfs and normal stars, also have strong magnetic fields that get even stronger the closer you get to the event horizon, or the point from which light cannot escape. For an introduction to degenerate matter, followed by a description the various stages of a stellar remnant's collapse preceding the possible formation of a black hole, see here. First, instead of conventional objects such as the earth and moon, they consider the production of black holes on white dwarfs and neutron stars. Now, researchers think they've got the solution — the burst of radiation could have been emitted by merger between superdense objects like black holes, white dwarfs or neutron stars. Black holes, neutron stars or white dwarfs, collided and merged together. Have you tried Black Holes, White Dwarfs, and Neutron Stars, by Shapiro and Teukolsky? Therefore, it is an ideal technique to study the galactic population of faint or dark objects, such as brown dwarfs, red dwarfs, white dwarfs, neutron stars, black holes and exoplanets. Sources of gravitational waves could possibly include binary star systems composed of white dwarfs, neutron stars, or black holes. We look at the skies and see stars at various stages of their evolution — young ones, middle aged ones, supernovas, and the remnants of supernovas — white dwarves, neutron stars, black holes. €This tell-tale signal, called a quasi-periodic oscillation or QPO, is a characteristic feature of the accretion disks that often surround the most compact objects in the universe — white dwarf stars, neutron stars and black holes. If a star has between 1.4 to 4 times our Sun's mass it will form a neutron star at its death. The satellite provided unprecedented views into the extreme environments around white dwarfs, neutron stars and black holes. They are extremely massive stars with a strong force of gravity.