This is the first comprehensive treatment of active galactic
nuclei--the cosmic powerhouses at the core of many distant
galaxies. The term "active galactic nuclei" refers to quasars,
radio galaxies, Seyfert galaxies, blazars, and related objects, all
of which are believed to share a similar central engine--a
supermassive black hole many times the mass of the Sun.
Astrophysicists have studied these phenomena for the past several
decades and have begun to develop a consensus about many of their
properties and internal mechanisms. Julian Krolik, one of the
world's leading authorities on the subject, sums up leading ideas
from across the entire range of research, making this book an
invaluable resource for astronomers, physicists interested in
applications of the theory of gravitation, and graduate
students.
Krolik begins by addressing basic questions about active
galactic nuclei: What are they? How can they be found? How do they
evolve? He assesses the evidence for massive black holes and
considers how they generate power by accretion. He discusses X-ray
and g-ray emission, radio emission and jets, emission and
absorption lines, anisotropic appearance, and the relationship
between an active nucleus and its host galaxy. He explores the
mysteries of what ignites, fuels, and extinguishes active galactic
nuclei, and concludes with a general review of where the field now
stands. The book is unique in paying careful attention to relevant
physics as well as astronomy, reflecting in part the importance of
general relativity to understanding active galactic nuclei. Clear,
authoritative, and detailed, this is crucial reading for anyone
interested in one of the most dynamic areas of astrophysics
today.
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