MCQC J162847-4152 - a Possible Brightest Microquasar found

Details MCQC J162847-4152 - a Possible Brightest Microquasar found MCQC J162847-4152 - a Possible Brightest Microquasar found

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001atel...80....1t&link_type=abstract

The Astronomer's Telegram, #80

Astronomy and Astrophysics

Astronomy

5

Radio, Millimeter, Infra-Red, Optical, X-Ray, Request For Observations, Binaries, Black Holes, Neutron Stars, Transients, Variables, Stars

Scientific paper

MCQC J162847-4152 is one of 40 objects found in the course of our systematic and complete survey for new microquasars in the whole Galactic plane (see project description in astro-ph/0110511). It is optically brightest and mostly definite microquasar candidate in the list, which we describe as follows: 1) It is a bright ROSAT source, 1RXS J162848.1-415241, in the Galactic plane (b=4.7deg), with a hard X-ray spectrum (HR1 = 1.00+/-0.04), which is characteristic of X-ray binaries (Motch et al., AAS 132, 341, 1998).

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