Counterparts to massive X-ray binaries

DOI

The X-ray and gamma-ray observatory INTEGRAL has discovered large numbers of new hard X-ray sources, many of which are believed to be high mass X-ray binaries. However, for a significant fraction, their counterparts remain unidentified. We explore the use of photometric catalogues to find optical counterparts to high mass X-ray binaries and search for objects likely to be early-type stars within the error circles of several INTEGRAL sources. *********** * * Sorry, but the author(s) never supplied the tabular material * announced in the paper * * ************

Identifier
DOI http://doi.org/10.26093/cds/vizier.34610631
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/461/631
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/461/631
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/461/631
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/461/631
Provenance
Creator Negueruela I.; Schurch M.P.E.
Publisher CDS
Publication Year 2007
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Physics; Stellar Astronomy