Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-01-17
Astronomy and Astrophysics
Astrophysics
In Proc. of ``Interacting Binaries: Accretion, Evolution, and Outcomes'', eds. L. A. Antonelli et al., AIP, Cefalu, Sicily, 20
Scientific paper
10.1063/1.2130261
We present results from the first near-IR imaging of the weak X-ray sources discovered in the Chandra/ACIS-I survey (Wang et al. 2002) towards the Galactic Centre (GC). These ~800 discrete sources, which contribute significantly to the GC X-ray emission, represent an important and previously unknown population within the Galaxy. From our VLT observations we will identify likely IR counterparts to a sample of the hardest sources, which are most likely X-ray binaries. With these data we can place constraints on the nature of the discrete weak X-ray source population of the GC.
Bandyopadhyay Reba M.
Bauer Franz Erik
Blundell Katherine M.
Miller-Jones James C. A.
Pfahl Eric
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