Microquasar candidates (Combi+, 2008)

Details Microquasar candidates (Combi+, 2008) Microquasar candidates (Combi+, 2008)

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34770125c&link_type=abstract

VizieR On-line Data Catalog: J/A+A/477/125. Originally published in: 2008A&A...477..125C

Physics

1

X-Ray Sources, Radio Sources, Infrared Sources, Qsos

Scientific paper

Microquasars are ideal natural laboratories for understanding accretion/ejection processes, studying the physics of relativistic jets, and testing gravitational phenomena. Nevertheless, these objects are difficult to find in our Galaxy. The main goal of this work is to increase the number of known systems of this kind, which should allow better testing of high-energy phenomena and more realistic statistical studies of this galactic population to be made.
We have developed an improved search strategy based on positional cross-identification with very restrictive selection criteria to find new MQs, taking advantage of more sensitive modern X-ray data. To do this, we made combined use of the radio, infrared, and X-ray properties of the sources, using different available catalogs.
(1 data file).

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