Analysis a new activity of the Be X-ray pulsar A0535+26

Details Analysis a new activity of the Be X-ray pulsar A0535+26 Analysis a new activity of the Be X-ray pulsar A0535+26

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010fym..confp..20n&link_type=abstract

"The First Year of MAXI: Monitoring Variable X-ray Sources", Poster Presentations, 4th International MAXI Workshop held November

Computer Science

Scientific paper

We report on the analysis results of the current X-ray activities of Be X-ray transient pulsar A0535+26 observed with MAXI/GSC. From 2009, the source again re-entered an active phase showing the periodic X-ray outbursts. In the current activities, the precursor events have been observed before the normal/giant outbursts. The present precursor and outburst period is to be 115-days instead of the 110-day orbital period. This difference would be related to the structure of the circumstellar disk of the companion Be star.

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