Swift/BAT confirms the outburst from 2S 1417-624

Details Swift/BAT confirms the outburst from 2S 1417-624 Swift/BAT confirms the outburst from 2S 1417-624

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2276....1k&link_type=abstract

The Astronomer's Telegram, #2276

Astronomy and Astrophysics

Astronomy

X-Ray, Binaries, Neutron Stars, Pulsars

Scientific paper

As part of its hard X-ray transient monitor program, the Burst Alert Telescope on Swift has detected a brightening of the high-mass X-ray binary and binary pulsar 2S 1417-624 which confirms the results recently reported from the Fermi/GBM (Beklen & Finger, ATel #2275). The source first became detectable on 14-Oct-2009, rising to a peak daily average brightness of 0.019 ± 0.002 counts/s/cm2, corresponding to ~85 mCrab in the 15-50 keV band, on 30-Oct-2009 (MJD 55134).

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