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


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




It's funny, because the more wacky combinations of stars and compact object (white dwarf, neutron star, or black hole) we find or imagine, the more remarkable evolutionary scenarios astronomers can conceive of playing out. It is thus an ideal technique to study the galactic population of such faint or dark objects as brown dwarfs, red dwarfs, planets, white dwarfs, neutron stars, black holes, and Massive Compact Halo Objects. Thumbnail of image, Near-infrared image of young binary stars with a faint companion (a planet?). 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. Short duration gamma-ray bursts are thought to be caused by the merger of some combination of white dwarfs, neutron stars or 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. An artist's impression of the merger of two neutron stars. Thumbnail, Image Description, Caption, NASA IDs, Image Size, Hi-Resolution TIFF? When stars die, the distribution of remnant masses would be expected to be continuous from white dwarfs through neutron stars to black holes, ranging from a fraction of our sun's mass to nearly 100 solar masses. 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. 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. If a star is much greater than 3 times our Sun's mass it will form a black hole at its death. €�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.

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