high-energy radiation from black holes: from supermassive black holes to galactic solar mass black...

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Preface High-Energy Radiation from Black Holes: From Supermassive Black Holes to Galactic Solar Mass Black Holes The 35th assembly of COSPAR in Paris in July 2004 included a meeting on ‘‘High-Energy Radiation from Black Holes: from Supermassive Black Holes to Galactic Solar Mass Black Holes’’. The meeting was designed to provide insights on observations and models of the close surround- ings of black holes in very different astrophysical contexts, including accreting binary systems, the center of our and other galaxies and active galactic nuclei. Observations cov- ering the electro-magnetic spectrum from the radio domain to gamma rays were presented and discussed. The meeting took place about 1.5 years after the launch of INTEGRAL and therefore allowed the authors to present new results in the hard X-ray domain. The meeting was very well attended and included many very high quality presentations that lead to interesting dis- cussions. This issue of Advances in Space Research presents a number of the contributions given during the conference. They are organised from galactic objects to extra galactic ones to surveys. The success of a meeting is always due to a large number of people. In the case of a COSPAR meeting during a gen- eral assembly, these include the organisers of the whole meeting. In Paris, the general assembly was a very lively and interesting gathering of space scientists in which several themes of interest to our community were well represented. This gave rise to constructive interferences between the participants of the various scientific meetings. The members of the scientific organising committee [T. Courvoisier (chair), P. Ubertini, J.-P. Roques, N. Lund, J. Paul, R. Mushotzky, J. Kaastra, B. Wilkes, K. Makishi- ma, R. Sunyaev, E. Churazov, A. King] provided very valuable help in designing an optimum programme. Clearly the value of the meeting is that given by the authors of the papers. We are very grateful to them for a set of brilliant contributions. The authors who chose to present their results in this issue also provided high quality manuscripts, for which they are warmly thanked. The papers presented here have been carefully peer reviewed by a number of astronomers including K. Beckwith, E. Churazov, L. Foschini, J. Paul, K. Pottschmidt, J. Rodriquez, R. Staubert, and M. Turler. We also thank them for their help in preparing this set of papers for pub- lication. The staff of COSPAR and Elsevier (in particular Peggy Ann Shea and Carmel Moloney), helped us find our way in the jungle of the edition process without ever loosing patience or temper; for this also we are grateful. Guest Editors T.J.-L. Courvoisier * INTEGRAL Science Data Centre, 16, Chemin d’Ecogia, 1290 Versoix, Switzerland E-mail address: [email protected] B. Wilkes Chandra X-ray Center Smithsonian Astrophysical Observatory, 60 Garden St., Cambridge, MA 02138, USA 0273-1177/$30 Ó 2006 Published by Elsevier Ltd on behalf of COSPAR. doi:10.1016/j.asr.2006.06.001 * Corresponding author. Tel.: +41 22 379 21 01; fax: +41 22 379 21 33. www.elsevier.com/locate/asr Advances in Space Research 38 (2006) 1345

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www.elsevier.com/locate/asr

Advances in Space Research 38 (2006) 1345

Preface

High-Energy Radiation from Black Holes: From SupermassiveBlack Holes to Galactic Solar Mass Black Holes

The 35th assembly of COSPAR in Paris in July 2004included a meeting on ‘‘High-Energy Radiation from BlackHoles: from Supermassive Black Holes to Galactic SolarMass Black Holes’’. The meeting was designed to provideinsights on observations and models of the close surround-ings of black holes in very different astrophysical contexts,including accreting binary systems, the center of our andother galaxies and active galactic nuclei. Observations cov-ering the electro-magnetic spectrum from the radio domainto gamma rays were presented and discussed. The meetingtook place about 1.5 years after the launch of INTEGRALand therefore allowed the authors to present new results inthe hard X-ray domain.

The meeting was very well attended and included manyvery high quality presentations that lead to interesting dis-cussions. This issue of Advances in Space Research presentsa number of the contributions given during the conference.They are organised from galactic objects to extra galacticones to surveys.

The success of a meeting is always due to a large numberof people. In the case of a COSPAR meeting during a gen-eral assembly, these include the organisers of the wholemeeting. In Paris, the general assembly was a very livelyand interesting gathering of space scientists in whichseveral themes of interest to our community were wellrepresented. This gave rise to constructive interferencesbetween the participants of the various scientific meetings.The members of the scientific organising committee[T. Courvoisier (chair), P. Ubertini, J.-P. Roques, N. Lund,

0273-1177/$30 � 2006 Published by Elsevier Ltd on behalf of COSPAR.

doi:10.1016/j.asr.2006.06.001

J. Paul, R. Mushotzky, J. Kaastra, B. Wilkes, K. Makishi-ma, R. Sunyaev, E. Churazov, A. King] provided veryvaluable help in designing an optimum programme.

Clearly the value of the meeting is that given by theauthors of the papers. We are very grateful to them for aset of brilliant contributions. The authors who chose topresent their results in this issue also provided high qualitymanuscripts, for which they are warmly thanked. Thepapers presented here have been carefully peer reviewedby a number of astronomers including K. Beckwith,E. Churazov, L. Foschini, J. Paul, K. Pottschmidt, J.Rodriquez, R. Staubert, and M. Turler. We also thankthem for their help in preparing this set of papers for pub-lication. The staff of COSPAR and Elsevier (in particularPeggy Ann Shea and Carmel Moloney), helped us findour way in the jungle of the edition process without everloosing patience or temper; for this also we are grateful.

Guest Editors

T.J.-L. Courvoisier *

INTEGRAL Science Data Centre,

16, Chemin d’Ecogia,

1290 Versoix, Switzerland

E-mail address: [email protected]

B. WilkesChandra X-ray Center Smithsonian

Astrophysical Observatory,

60 Garden St., Cambridge, MA 02138, USA

* Corresponding author. Tel.: +41 22 379 21 01; fax: +41 22 379 21 33.