IGR J17418-1212 - A Possible Microquasar with Multiple Identification

Details IGR J17418-1212 - A Possible Microquasar with Multiple Identification IGR J17418-1212 - A Possible Microquasar with Multiple Identification

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..239....1t&link_type=abstract

The Astronomer's Telegram, #239

Astronomy and Astrophysics

Astronomy

3

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

Scientific paper

Due to Bassani et al., ATEL #232/, the source No. 5 = IGR J17418-1212 (b = 9.4 deg.) was first detected in the hard X-ray band (>20 keV) by the IBIS/ISGRI instrument of INTEGRAL, and is probably identified with 2E1739.1-1210. I call attention that the INTEGRAL object coincides unambiguously with the bright ROSAT source 1RXS J174155.3-121157.

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