Swift/BAT detects renewed hard X-ray activity from pulsar XTE J1858+034

Details Swift/BAT detects renewed hard X-ray activity from pulsar XTE J1858+034 Swift/BAT detects renewed hard X-ray activity from pulsar XTE J1858+034

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2846....1k&link_type=abstract

The Astronomer's Telegram, #2846

Astronomy and Astrophysics

Astronomy

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

Scientific paper

The Swift/BAT hard X-ray transient monitor reports renewed activity in the 15-50 keV band for the transient X-ray pulsar and high mass X-ray binary system XTE J1858+034. Starting on 2010-Sep-14 (MJD 55453), the source has increased in intensity from an undetectable level (one-sigma upper limit of 0.0027 cts/cm2/sec or 12 mcrab) up to a current level of 0.012 ± 0.0038 cts/cm2/sec (50 mcrab) on 2010-Sep-17.

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