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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
Publisher: John Wiley & Sons Inc
Page: 653
ISBN: 0471873179, 9780471873174
Format: djvu

Short duration gamma-ray bursts are thought to be caused by the merger of some combination of white dwarfs, neutron stars or black holes. Translated with Secret Alien Technology: Alien here,. An exhausted star will evolve into a neutron star, a black hole or a white dwarf – depending on its mass. €�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. Black Holes, Neutron Stars, White Dwarfs, Space and Time. An artist's impression of the merger of two neutron stars. Lately, I've been asked several questions about space travel. Vocabulary to remember: nebula, protostar, hydrostatic equilibrium, thermonuclear reaction, main-sequence star, red giant, supernova, black holes, white dwarf, neutron star. Have you tried Black Holes, White Dwarfs, and Neutron Stars, by Shapiro and Teukolsky? Answer to previous quiz (click here) Option D- (All of the above) "The ultimate fate of the star whether it is a white dwarf, Neutron star or a Black Hole depends on its initial mass. Sources of detectable gravitational waves could possibly include binary star systems composed of white dwarfs, neutron stars, or 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. A star undergoes many radical changes throughout its lifespan including the inevitable exhaustion of its fuel source. Neutron star simulation in Astrophysics is being discussed at Physics Forums. What does a black hole look like?