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Publisher:
Cambridge University Press
Online publication date:
August 2010
Print publication year:
1994
Online ISBN:
9780511564765

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.

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Contents


Page 3 of 4


  • Dramatic X-ray Spectral Variability of Mkn 841
    pp 278-279
    • By Ian M. George, Laboratory for High Energy Astrophysics, Code 668, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A., and Universities Space Research Association, Paul Nandra, Institute of Astronomy, Magingley Road, Cambridge, CB3 0HA, U.K., Andy C. Fabian, Institute of Astronomy, Magingley Road, Cambridge, CB3 0HA, U.K., T. Jane Turner, Laboratory for High Energy Astrophysics, Code 668, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A., and Universities Space Research Association, Chris Done, X-ray Astronomy Group, Department of Physics & Astronomy, University of Leicester, Leicester, LEI 7RH, U.K., Chas S.R. Day, Laboratory for High Energy Astrophysics, Code 668, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A., and Universities Space Research Association

Page 3 of 4


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