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 astrophysicstoday.