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Black holes, white dwarfs, and neutron stars epub

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

Black holes, white dwarfs, and neutron stars


Black.holes.white.dwarfs.and.neutron.stars.pdf
ISBN: 0471873179,9780471873174 | 653 pages | 17 Mb


Download Black holes, white dwarfs, and neutron stars



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




Royal Astronomical Society that suggest that two “compact stellar remnants” — which could be neutron stars, black holes or white dwarfs — collided and merged, resulting in a short-duration gamma-ray burst that hit Earth. They suggest that two compact stellar remnants – black holes, neutron stars or white dwarfs – collided and merged together. We call this type of explosion a "Type Ia supernova" ("Type Ia" is a historical moniker from before we understood what was exploding), and the supernova completely obliterates the white dwarf. Lectures will be presented by leading Physicists and Astrophysicists working in the interface of Nuclear Physics, White Dwarfs, Neutron Star Physics and Black Holes Physics. Vocabulary to remember: nebula, protostar, hydrostatic equilibrium, thermonuclear reaction, main-sequence star, red giant, supernova, black holes, white dwarf, neutron star. White dwarfs, neutron stars, black holes, X-ray pulsars you name it and this book has it. Brown Dwarfs, is a fourth, remnant of a dead star after White Dwarfs, Neutron Stars, and Black Holes. In all it gives This is an exciting account about binary stars and the way black holes, white dwarfs, and neutron stars can evolve in them. Brown Dwarfs, in theory, have been around awhile, but the first to be discovered came in 1995. If a star has between 1.4 to 4 times our Sun's mass it will form a neutron star at its death. If a star is much greater than 3 times our Sun's mass it will form a black hole at its death. 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. 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. The white dwarf-neutron star final remnant consists of a cold neutron star core with a hot mantle on top.

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