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Supermassive Black Holes in the Distant Universe (Paperback, Softcover reprint of hardcover 1st ed. 2004)
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Supermassive Black Holes in the Distant Universe (Paperback, Softcover reprint of hardcover 1st ed. 2004)
Series: Astrophysics and Space Science Library, 308
Expected to ship within 10 - 15 working days
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Quasars, and the menagerie of other galaxies with "unusual nuclei,"
now collectively known as Active Galactic Nuclei or AGN, have, in
one form or another, sparked the interest of astronomers for over
60 years. The only known mechanism that can explain the staggering
amounts of energy emitted by the innermost regions of these systems
is gravitational energy release by matter falling towards a
supermassive black hole --- a black hole whose mass is millions to
billions of times the mass of our Sun. AGN emit radiation at all
wavelengths. X-rays originating at a distance of a few times the
event horizon of the black hole are the emissions closest to the
black hole that we can detect; thus, X-rays directly reveal the
presence of active supermassive black holes. Oftentimes, however,
the supermassive black holes that lie at the centers of AGN are
cocooned in gas and dust that absorb the emitted low energy X-rays
and the optical and ultraviolet light, hiding the black hole from
view at these wavelengths. Until recently, this low-energy
absorption presented a major obstacle in observational efforts to
map the accretion history of the universe. In 1999 and 2000, the
launches of the Chandra and XMM-Newton X-ray Observatories finally
broke the impasse. The impact of these observatories on X-ray
astronomy is similar to the impact that the Hubble Space Telescope
had on optical astronomy. The astounding new data from these
observatories have enabled astronomers to make enormous advances in
their understanding of when accretion occurs."
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