Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0128d&link_type=abstract
American Astronomical Society, HEAD meeting #9, #1.28; Bulletin of the American Astronomical Society, Vol. 38, p.333
Astronomy and Astrophysics
Astronomy
Scientific paper
We report here on near infrared observations of the field around IGR J16358-4756. The source belongs to the new class of highly absorbed X-ray binaries discovered by IBIS/INTEGRAL. Our primary goal was to identify the infrared counterpart of the source, previously suggested to be a LMXB and then further reclassified as a HMXB. We have made use of Chandra observations of the source in order to better constrain the number of possible counterparts. Using the differential photometry technique, in observations spanning a timescale of 1 month, we found no long term variability in our observations. This is compatible, and we suggest here, that the source is a HMXB.
Cieslinski Deonisio
D'Amico Flavio
Hickel Gabriel R.
Jablonski Francisco
Rodrigues Claudia Vilega
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