Fermi GBM Detection of Renewed Activity from 4U 0115+63

Details Fermi GBM Detection of Renewed Activity from 4U 0115+63 Fermi GBM Detection of Renewed Activity from 4U 0115+63

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3745....1j&link_type=abstract

The Astronomer's Telegram, #3745

Astronomy and Astrophysics

Astronomy

X-Ray, Binary, Neutron Star, Pulsar

Scientific paper

We report on renewed X-ray activity from Be/X-ray binary pulsar 4U 0115+63 observed with Fermi/GBM. Pulsation in the 8-25 keV band were first observed in the November 4.0-6.0 time interval, with a frequency of 276.69070(34) mHz. This measurement is orbitally corrected using ephemeris from Bildsten et. al (1997). The rms pulse flux rose to 15 mCrab in the 8-25 keV band on November 6. This source was last active in October 2011 (ATel #3677), during the previous orbit, for which we detected the source from October 11-18.

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