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X-ray Astronomy '999
Stellar Endpoints, AGN and the Diffuse Background
CNR - Conference Centre
Bologna - Italy
September 6-10, 1999

Organized by
ITESRE/CNR
and
NASA Goddard Space Flight Center

GSFC conference web site in the USA

Aug 2001 URGENT NOTICE
about X-ray Astronomy 1999 proceedings

List of Participants, Scientific Programme, Proceedings
BHs could be source of half of Universe's energy

X-ray Binaries and the X-ray background were the first two classes of cosmic X-ray source discovered. The X-ray binaries provide a natural laboratory for probing the extreme environments of black holes and neutron stars. A substantial fraction of the X-ray background is the superposition of AGN, which are powered by supermassive black holes. The Symposium will in two parts present observations from ASCA, ChandraAXAF, BeppoSAX, CGRO, ROSAT, and RossiXTE and ABRIXAS and will discuss their implications for the origin of the X-ray background and models for accretion on all scales.

Scientific Programme

Proceedings

Registration & Abstract Submission

Hotel booking form

How to reach Bologna CNR Area

1st Circular (Jan 1999)

2nd Circular (Apr 1999)

Scientific Organizing Committee (SOC)

N. White (GSFC) - chair

Compact Objects AGN & the XRB
D. Barret (Toulouse) N. Brandt (Penn State)
L. Bildsten (Berkeley) X. Barcons (Cantabria)
G. Di Cocco (Bologna) T. Courvoisier (Geneva)
F. Haberl (MPE) G. Hasinger (AIP)
N. Kawai (Riken) A. Fabian (IOA)
M. van der Klis (Amsterdam) T. Maccacaro (Brera, Milan)
S. Kulkarni (CalTech) G.G.C. Palumbo (Bologna)
F. Nagase (ISAS) L. Piro (Rome)
F. Paerels (Utrecht) H. Tananbaum (CFA)
A. Parmar (ESTEC) J. Turner (UMBC)
L. Stella (Rome Observatory) M. Urry (STScI)
R. Sunyaev (IKI & MPA) M. Ward (Leicester)

Local Organizing Committee (LOC)

G. Malaguti (Chair), L. Bassani, M. Cappi, A. Comastri, D. Dal Fiume, M. Orlandini, E. Palazzi, E. Pian, A. Spizzichino

For any information contact the local organizing committee at bo99@tesre.bo.cnr.it

 


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This file was last modified on by Pino Malaguti