Further observations of GRO J1750-27 (AX J1749.1-2639) with INTEGRAL

Details Further observations of GRO J1750-27 (AX J1749.1-2639) with INTEGRAL Further observations of GRO J1750-27 (AX J1749.1-2639) with INTEGRAL

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1400....1b&link_type=abstract

The Astronomer's Telegram, #1400

Astronomy and Astrophysics

Astronomy

2

X-Ray, Gamma Ray, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

The transient accreting X-ray pulsar GRO J1750-27 (AX J1749.1-2639), which became active end of January 2008 (ATel #1376), has been repeatedly observed by the INTEGRAL Galactic Bulge monitoring program since mid February (ATel #1385) on 11, 20 and 23 Feb. 2008. During the three observations, totalling about 27 ks, the source has remained bright at a roughly constant level with the following flux averaged over the 3 observations: 186+/-9 mCrab (3-10 keV), 319+/-15 mCrab (10-25 keV), 198+/-2 mCrab (18-40 keV), and 20+/-3 mCrab (40-100 keV).

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