LMXBs in the bulge of M31

DOI

We explore the population of X-ray point sources in the bulge of M31 to contrast properties of various subpopulations, such as persistent and transient sources and primordial LMXBs and dynamically formed ones. Based on the data from 26 archival Chandra observations we study the source content and properties of various subpopulations of X-ray sources to a maximum distance of 12' from the centre of M 31.

Cone search capability for table J/A+A/468/49/table2 (The list of point like X-ray sources within a distance of 12' from the centre of M 31.)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34680049
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/468/49
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/468/49
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/468/49
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/468/49
Provenance
Creator Voss R.; Gilfanov M.
Publisher CDS
Publication Year 2008
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; Galactic and extragalactic Astronomy; Natural Sciences; Physics; Stellar Astronomy