Upcoming Meetings - GCNEWS, Vol. 26, April 2007
GCNEWS
A Newsletter for Galactic Center Research
Currently edited by Sera Markoff, Loránt Sjouwerman,
Joseph Lazio, Cornelia Lang, Rainer Schödel, Masaaki
Sakano & Feng Yuan
email: gcnews@aoc.nrao.edu
Volume 26, April 2007
- Upcoming Meetings
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Bursts, Pulses and Flickering:
Wide-Field Monitoring of the Dynamic Radio Sky
June 12-15 2007, Kerastari, Greece
Final details
We included the full announcement last issue, but just a reminder that
the registration and hotel booking is open in April, with
pre-registration encouraged. Please see the webpage for more details:
http://www.atnf.csiro.au/Dynamic2007/
GC2007: Celebrating 15 years of Precision Astronomy in the Galactic
Center - Hot Topics and Observational Challenges
June 17-23, 2007, Ringberg Castle, Germany
In 1992, the first observations of a star in a close orbit around the
supermassive blackhole at the Galactic Center were obtained. Today we
know that this star, "S2", has a period of 15 years, so 2007 we can
celebrate the first revolution of "S2". We are doing so by organizing
a scientific workshop to be held at Schloss Ringberg (Ringberg
castle), Bavaria (http://www.schloss-ringberg.de). The main focus of
the conference will be stellar dynamics in the Galactic Center. A full
day will also be dedicated to the topic of Sgr A*. Because
accomodation is limited to 65, the meeting will not have an open
registration. For more details see the conference website:
http://www.mpe.mpg.de/ir/meetings/ringberg2007/index.php
SOC: Tal Alexander, Fred Baganoff, Marcella Carollo, Andreas Eckart,
Heino Falcke, Karl Gebhardt, Reinhard Genzel (Chair), Ortwin Gerhard,
Andrea Ghez, Abraham Loeb, Mark Morris, Eliot Quataert, Mark Reid,
Daniel Rouan, Jonathan Tan
A Population Explosion: The Nature and Evolution of X-ray Binaries in Diverse Environments
October 28-November 2 2007, St. Petersburg Beach, FL
In recent years, technological advances in X-ray astronomy have led to
the discovery of a large number of previously undetected high-energy
sources, increasing by an order of magnitude the known population of
X-ray binaries in the Galaxy. This meeting will address the current
state of observational and theoretical research into the X-ray binary
population as a whole, incorporating studies of both the previously
known, well-studied systems and the newly discovered populations, and
examine the feedback and interaction of X-ray binaries with their
environment within our own Galaxy and in external galaxies. We would
especially like to highlight research on recently discovered
populations of accreting binaries, including the faint hard X-ray
sources in the Galactic Centre, obscured sources identified with
INTEGRAL, supergiant fast X-ray transients, and extragalactic
binaries.
We have established five major topics for this five-day conference, and plan to devote one day to each topic:
- X-ray binary jets at high and low luminosities, and their effect on the XRB environment
- Faint X-ray binary populations, especially the in Galactic Centre
- Obscured populations (INTEGRAL sources, SFXTs)
- Extragalactic X-ray binary populations and ULXs
- X-ray binary population synthesis and stellar evolution
SOC: Stefanie Wachter (Spitzer Science Center/Caltech), Reba
Bandyopadhyay (University of Florida) (co-chairs), Sera Markoff (University of
Amsterdam) Jocelyn Bell Burnell (University of Oxford), Philipp
Podsiadlowski (University of Oxford), Tom Maccarone (University of
Southampton), Rob Fender (University of Southampton), Michael Muno
(Caltech), John Tomsick (University of California, Berkeley), Saku
Vrtilek (Harvard/CfA), Phil Charles (SAAO)
The deadline for registration and submitting abstracts is 1 June 2007,
using the secure server on the conference website:
http://conference.astro.ufl.edu/XRAYBIN/
Attendance at the meeting will be limited to 170 participants. For
more details see the webpages.
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File last modified on Friday 20 April 2007 [16:41 MDT].
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