MAXI GSC detection of a renewed X-ray activity from Be X-ray binary pulsar XTE J1858+034

Details MAXI GSC detection of a renewed X-ray activity from Be X-ray binary pulsar XTE J1858+034 MAXI GSC detection of a renewed X-ray activity from Be X-ray binary pulsar XTE J1858+034

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3766....1s&link_type=abstract

The Astronomer's Telegram, #3766

Astronomy and Astrophysics

Astronomy

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

Scientific paper

We report on the renewed X-ray activity of a Be/X-ray binary pulsar, XTE J1858+034 observed with MAXI/GSC. The source flux in 4-10 keV band was 12 ± 5 mCrab in one-day average on 2011 November 6 (MJD 55871), and slowly increased up to 24 ± 5 mCrab on November 15 (MJD 55880). The flux in 2-4 keV has been <10 mCrab at the 1-sigma upper limit for these period, which indicates that the source is moderately absorbed.

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