Rapid Brightening of A0535+26 Observed by Fermi GBM

Details Rapid Brightening of A0535+26 Observed by Fermi GBM Rapid Brightening of A0535+26 Observed by Fermi GBM

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2324....1w&link_type=abstract

The Astronomer's Telegram, #2324

Astronomy and Astrophysics

Astronomy

10

X-Ray, Gamma Ray, Binaries, Pulsars, Transients

Scientific paper

A0535+262 is brightening rapidly in GBM observations. On November 30, 2009, Fermi GBM Earth occultation observations showed that the flux had risen rapidly to 480+/-100, 460+/-70, and 620+/-100 mCrab in the 8-12, 12-25, and 25-50 keV bands. On December 1, 2009 the flux continued to rise to 580+/-105, 640+/-50, 444+/-80 mCrab in the 8-12,12-25, and 25-50 keV bands respectively. After remaining fairly constant at 10 mCrab from November 19-24, the pulsed rms flux in the 12-50 keV band began to rise, reaching 70 mCrab on December 1.

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