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SAX J2103.5+4545 in outburst

By Galis, R.; Beckmann, V.; Bianchin, V.; Grebenev, S.; McBreen, B.; Mereghetti, S.; Revnivtsev, M.; Sanchez, C.; Strong, A.; Westergaard, N. J.1

From

National Space Institute, Technical University of Denmark1

We report an intense hard X-ray outburst detected from the Be/ neutron star HMXB SAX J2103.5+4545 (Blay et al. 2004, A&A, 427, 293), which is known to be a pulsar. The source was detected during INTEGRAL observations of the Galactic Plane in the Cygnus region, starting at 2007-04-25T09:14 (UTC). The source was detected by INTEGRAL IBIS/ISGRI within 60 ksec with a flux of (1.7 +- 0.1)E-09 erg/cm**2/sec in the 20-40 keV energy band, and with (5.3 +- 0.7)E-10 erg/cm**2/sec at 40-80 keV.

Language: English
Year: 2008
Types: Other
ORCIDs: Westergaard, N. J.
Keywords

Binary Neutron star Pulsar X-ray

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