Supermassive Black Holes in the Distant Universe

  • Amy J. Barger

Part of the Astrophysics and Space Science Library book series (ASSL, volume 308)

Table of contents

  1. Front Matter
    Pages i-x
  2. Richard Mushotzky
    Pages 53-87
  3. Zoltán Haiman, Eliot Quataert
    Pages 147-185
  4. Guido Risaliti, Martin Elvis
    Pages 187-224
  5. Lennox L. Cowie, Amy J. Barger
    Pages 273-298
  6. Back Matter
    Pages 299-304

About this book


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.


Accretion Galaxy Observatories Quasar Universe

Editors and affiliations

  • Amy J. Barger
    • 1
    • 2
    • 3
  1. 1.Department of AstronomyUniversity of Wisconsin-MadisonUSA
  2. 2.Department of Physics and AstronomyUniversity of HawaiiHonoluluUSA
  3. 3.Institute for AstronomyUniversity of HawaiiHonoluluUSA

Bibliographic information

  • DOI
  • Copyright Information Springer Science+Business Media B.V. 2004
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Print ISBN 978-90-481-6662-6
  • Online ISBN 978-1-4020-2471-9
  • Series Print ISSN 0067-0057
  • Buy this book on publisher's site