MAXI/GSC detects re-brightening of Be pulsar A0535+262

Details MAXI/GSC detects re-brightening of Be pulsar A0535+262 MAXI/GSC detects re-brightening of Be pulsar A0535+262

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2754....1n&link_type=abstract

The Astronomer's Telegram, #2754

Astronomy and Astrophysics

Astronomy

1

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

Scientific paper

An increase of X-ray flux of the Be/X-ray binary pulsar A0535+26 was observed with MAXI/GSC on 2010 July 17 at 21+-5 mCrab (2-20 keV). This is the fourth detection of the consecutive outbursts following the 111 day orbital cycle. After the detection by Fermi GBM (ATel #2705) on June 25, which is probably the precursor of the fourth outburst in the series, its flux once decreased below 20 mCrab on July 11 (MJD 55388).

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