Active Galactic Nuclei: From the Central Black Hole to the Galactic Environment
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.

1101639783
Active Galactic Nuclei: From the Central Black Hole to the Galactic Environment
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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Active Galactic Nuclei: From the Central Black Hole to the Galactic Environment

Active Galactic Nuclei: From the Central Black Hole to the Galactic Environment

by Julian H. Krolik
Active Galactic Nuclei: From the Central Black Hole to the Galactic Environment

Active Galactic Nuclei: From the Central Black Hole to the Galactic Environment

by Julian H. Krolik

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Overview

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.


Product Details

ISBN-13: 9780691011516
Publisher: Princeton University Press
Publication date: 01/10/1999
Series: Princeton Series in Astrophysics , #59
Pages: 632
Product dimensions: 6.00(w) x 9.00(h) x (d)

About the Author

Julian H. Krolik is Professor of Physics and Astronomy at The Johns Hopkins University. He has written widely on theoretical astrophysics, specializing in active galactic nuclei.

Table of Contents

Preface
Guide for Readers
1What Are Active Galactic Nuclei? And Why Does Anyone Care?3
2How to Find AGNs22
3Evolution42
4Global Energetics and Black Holes68
5Black Hole Physics90
6Spherical Accretion120
7Accretion Disks and the Optical/Ultraviolet Continuum135
8X-ray and [gamma]-ray Emission196
9Radio Emission and Jets256
10Emission Lines309
11Intrinsic Absorption and Outflows399
12Anisotropic Appearance and Unification of Disparate AGN Varieties424
13Properties of AGN Host Galaxies464
14Onset and Fueling494
15Where We Stand530
App. ABasic General Relativity533
App. BBasic Magnetohydrodynamics537
App. CShocks and Other Discontinuities542
App. DLuminosity Functions and Other Population Statistics552
App. EThe Tensor Viral Theorem559
App. FKinematics in an Expanding Universe566
References573
Index589

What People are Saying About This

Marek Abramowicz

I read this book with great interest and joy. It covers the whole subject of active galactic nuclei in depth.
Marek Abramowicz, Goteborg University, Sweden

From the Publisher

"Julian Krolik, himself a substantial contributor to high-energy astrophysics, has written an impressive book that will be welcomed by researchers in the field. . . . It fills a notable gap in the existing literature."—Martin Rees, Institute of Astronomy, University of Cambridge

"I read this book with great interest and joy. It covers the whole subject of active galactic nuclei in depth."—Marek Abramowicz, Göteborg University, Sweden

Martin Rees

Julian Krolik, himself a substantial contributor to high-energy astrophysics, has written an impressive book that will be welcomed by researchers in the field. . . . It fills a notable gap in the existing literature.
Martin Rees, Institute of Astronomy, University of Cambridge

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