Skip to main content Accessibility help

We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.

Close cookie message
×
  1. Home
  2. Books
  3. The Nature of Compact Objects in Active Galactic Nuclei
Publisher:
Cambridge University Press
Online publication date:
August 2010
Print publication year:
1994
Online ISBN:
9780511564765
DOI:
https://doi.org/10.1017/CBO9780511564765
Subjects:
Physics and Astronomy, Astrophysics
Information

Book description

What evidence is there for and against unified schemes for active galactic nuclei (AGN)? How do the AGN populations evolve over cosmological timescales? And what can the variability of their UV and X-ray emission tell us? These are just some of the exciting issues addressed in this volume of papers collected from the 33rd Herstmonceux conference in Cambridge. AGN are among the most spectacular objects known to astronomy. Yet, despite years of intense and wide-ranging research, the debate continues - what is their fundamental source of power? Rapid progress has been made towards answering this question by a variety of large-scale, multi-wavelength monitoring campaigns and the latest generation of satellite-borne observations. This volume provides a valuable overview and timely update of the exciting and rapidly developing field of AGN research - essential reading for graduate students and researchers.

Refine List

Actions for selected content:

Select all | Deselect all
  • View selected items
  • Export citations
  • Download PDF (zip)
  • Save to Kindle
  • Save to Dropbox
  • Save to Google Drive

Save Search

You can save your searches here and later view and run them again in "My saved searches".

Please provide a title, maximum of 40 characters.
Cancel
×

Contents

Page 1 of 4

Contents
  • Imaging Spectrophotometry of Extended-Emission Seyfert Galaxies
    pp 36-39
    • By Richard W. Pogge, Department of Astronomy, Ohio State University, Columbus, OH 43210, USA., Visiting Astronomers, Canada-France-Hawaii Telescope, operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique de France, and the University of Hawaii., Michael M. DeRobertis, Department of Physics and Astronomy, York University, North York, Ontario M3J 1P3, Canada, Visiting Astronomers, Canada-France-Hawaii Telescope, operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique de France, and the University of Hawaii.
  • Collimated Radiation in NGC 4151
    pp 46-47
    • By G. Kriss, Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218., I. Evans, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218., H. Ford, Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218., Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218., Z. Tsvetanov, Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218., A. Davidsen, Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218., A. Kinney, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218.
  • The Radio-Optical Connection in AGN
    pp 66-73
    • By David J. Axon, Affiliated with the Space Science Division of ESA at the Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD, USA and Nuffield Radio Astronomy Laboratory, University of Manchester, Jodrell Bank, Macclesfield, Cheshire, England, J. E. Dyson, Department of Astronomy, University of Manchester, Oxford road, Manchester, England., Alan Pedlar, Nuffield Radio Astronomy Laboratory, University of Manchester, Jodrell Bank, Macclesfield, Cheshire, England.

Page 1 of 4

Metrics

Full text views

Total number of HTML views: 0
Total number of PDF views: 0 *
Loading metrics...

Book summary page views

Total views: 0 *
Loading metrics...

* Views captured on Cambridge Core between #date#. This data will be updated every 24 hours.

Usage data cannot currently be displayed.