High
Energy View of Accreting Objects: AGN and X-ray Binaries
Agios Nikolaos, Crete, Greece
5 - 14 October 2010
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The presentations are available here Scientific Rationale:
The
rationale for this
conference is to bring together experts in the physics of accreting
objects (and their environments) at
all mass scales, from stellar to AGN, to discuss critically the main,
still open, issues related to the high-energy
manifestation of these phenomena, such as:
- Accretion modes versus accretor mass
- Inflows vs outflows
- Feedback
- Unification schemes
- States
and state transitions in
neutron-star and black-hole binaries
- Timing
(QPO, ms, kHz) and broad-band
spectral variability in X-ray binaries
- Jet-disk
connection in black hole
binaries
- Compact X-ray source populations in our Galaxy and other galaxies
|
AGNs:
M.
Begelman
S. Bianchi A. Comastri D. Crenshaw B. Czerny M. Elvis Y. Krongold A. Laor S. Mathur I. McHardy G. Miniutti R. Mushotzky M. Page J. Reeves N. Schartel J. Turner M. Watson |
X-ray Binaries: T.
Belloni
J. Casares M.J. Coe T. di Salvo C. Done P. Fabbiano F. Haberl V. Kalogera E. Koerding T. Maccarone I. McHardy R. Narayan I. Negueruela J.M. Paredes A. Papitto T. Roberts M. van der Klis |
Scientific Organizing Committee:
M. Elvis, B. Czerny, P. Nandra, F. Nicastro, M. Coe, T. Belloni, C. Done, P. Reig.
Local Organizing Committee:
P. Bonfini, O. Gonzalez-Martin, N. Kylafis, G. Maravelias, F. Nicastro, I. Papadakis, P. Reig, A. Zezas.
This
conference is
sponsored by the project GA No. 206469 (REGPOT-2007-1)
of the Seventh Framework Programme for Research and Technological
Development of the European Union.
