Swift observations of the continuing outburst of GRO J1750-27

Details Swift observations of the continuing outburst of GRO J1750-27 Swift observations of the continuing outburst of GRO J1750-27

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1401....1p&link_type=abstract

The Astronomer's Telegram, #1401

Astronomy and Astrophysics

Astronomy

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

Scientific paper

The current outburst of the accretion powered pulsar GRO J1750-27 (AX J1749.1-2639), first detected by Swift BAT on 2008 January 29 (ATEL#1376) and observed during the INTEGRAL Galactic Bulge monitoring (ATEL#1385, ATEL#1400), is continuing. The BAT light curve shows a stable level of emission at ~250 mCrab in the 15-50 keV band, see http:// swift.gsfc.nasa.gov/docs/swift/results/transients/weak/AXJ1749.1-2639/.

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