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An Infrared Imaging Survey of the Faint Chandra Sources near the Galactic Centre

Abstract:
We present near-IR imaging of a sample of the faint, hard X-ray sources discovered in the 2001 Chandra ACIS-I survey towards the Galactic Centre (GC) (Wang et al. 2002). These ~800 discrete sources represent an important and previously undetected population within the Galaxy. From our VLT observations of 77 X-ray sources, we identify candidate K-band counterparts to 75% of the Chandra sources in our sample. The near-IR magnitudes and colours of the majority of candidate counterparts are consistent with highly reddened stars, indicating that most of the Chandra sources are likely to be accreting binaries at or near the GC.
Publication status:
Published

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Publisher copy:
10.1111/j.1365-2966.2005.09607.x

Authors

More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
364
Issue:
4
Pages:
1195-1202
Publication date:
2005-09-13
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
Pubs id:
pubs:3145
UUID:
uuid:f3210a13-9c39-4342-9768-22185cc1a27c
Local pid:
pubs:3145
Source identifiers:
3145
Deposit date:
2012-12-19
ARK identifier:

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