pith. sign in

arxiv: 1009.2454 · v1 · pith:35ECY26Tnew · submitted 2010-09-13 · 🌌 astro-ph.HE

Sample of LMXBs in the Galactic bulge. I. Optical and near-infrared constraints from the Virtual Observatory

classification 🌌 astro-ph.HE
keywords opticalbulgeconstraintsdataestimatesgalacticnear-infraredobjects
0
0 comments X
read the original abstract

We report on the archival optical and near-infrared observations of 6 low mass X-ray binaries situated in the Galactic bulge. We processed several recent Chandra and XMM-Newton as well as Einstein datasets of a binary systems suspected to be ultracompact, which gave us arcsec-scale positional uncertainty estimates. We then undertook comprehensive search in existing archives and other Virtual Observatory resources in order to discover unpublished optical/NIR data on these objects. We found and analysed data from ESO Archive and UKIRT Infrared Deep Sky Survey (UKIDSS) on SLX 1735-269, 3A 1742-294, SLX 1744-299, SLX 1744-300, GX 3+1, IGR J17505-2644 systems and publish their finding charts and optical flux constraints in this paper, as well as simple estimates of the physical parameters of these objects.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.