Swift/BAT confirms renewed hard X-ray activity from pulsar SAX J2103.5+4545

Details Swift/BAT confirms renewed hard X-ray activity from pulsar SAX J2103.5+4545 Swift/BAT confirms renewed hard X-ray activity from pulsar SAX J2103.5+4545

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2928....1k&link_type=abstract

The Astronomer's Telegram, #2928

Astronomy and Astrophysics

Astronomy

X-Ray, Binary, Neutron Star, Transient, Pulsar

Scientific paper

The Swift/BAT hard X-ray transient monitor reports renewed hard X-ray activity in the 15-50 keV band from the Be/X-ray pulsar binary system SAX 2103.5+454. This confirms the X-ray activity predicted for this source by Kiziloglu et al. (ATel #2925). Starting on 2010-Oct-10 (MJD 55479), the source has increased in intensity from an undetectable level (one- sigma upper limit of 0.0007 cts/cm^2/sec or 3 mcrab) up to a level of 0.0073 ± 0.0010 cts/cm^2/sec (30 mcrab) on 2010-Oct-12.

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