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Black holes, white dwarfs, and neutron stars by Saul A. Teukolsky, Stuart L. Shapiro

Black holes, white dwarfs, and neutron stars Saul A. Teukolsky, Stuart L. Shapiro ebook
Page: 653
Format: djvu
ISBN: 0471873179, 9780471873174
Publisher: John Wiley & Sons Inc

They suggest that two compact stellar remnants – black holes, neutron stars or white dwarfs – collided and merged together. For 16 years NASA's Rossi X-ray Timing Explorer, RXTE to his friends, provided unprecedented views into the hearts of black holes, white dwarfs and neutron stars. An artist's impression of the merger of two neutron stars. 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. Short duration gamma-ray bursts are thought to be caused by the merger of some combination of white dwarfs, neutron stars or black holes. Shows the central region of our Milky Way galaxy, only about 25,000 light years from Earth, revealing hundreds of white dwarf stars, neutron stars, and black holes bathed in an incandescent fog of multimillion-degree gas. The trio would thereby be sensitive to the gravitational waves produced by small, dense objects orbiting one another, objects like white dwarfs, neutron stars and, most excitingly, black holes. This includes white dwarf stars, neutron stars and black holes. Chandra also finds regions aglow with the light of massive young stars. Possible MACHOs include faint white dwarfs, neutron stars, isolated black holes, and substellar objects such as brown dwarfs or free floating giant planets. Most of the material that formed the star is ejected into space in a supernova explosion, but the core of the star collapses to form a compact remnant which must be a white dwarf, a neutron star or a black hole. €�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. In the case of compact objects such as white dwarfs, neutron stars, and black holes, the gas in the inner regions becomes so hot that it will emit vast amounts of radiation (mainly X-rays), which may be detected by telescopes. 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. It finds a sea of hot gas enveloping thousands of white dwarfs, neutron stars and black holes. Black holes, white dwarfs, neutron stars and quasars emit an extremely strong, pulsing beam of Light, which is made up of the spectrum of Light waves that include Ultra-Violet.