4U 1901+03 observations with Fermi/GBM

Details 4U 1901+03 observations with Fermi/GBM 4U 1901+03 observations with Fermi/GBM

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3839....1j&link_type=abstract

The Astronomer's Telegram, #3839

Astronomy and Astrophysics

Astronomy

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

Scientific paper

Pulsations from the HMXB 4U 1901+3 are currently being detected with Fermi/GBM in the 8-25 keV band with a period near 2.762 s. The current outburst was previously reported by Sootome et al. (ATel #3829). We first detected this source on December 20. Observations from December 20 - 29 are inconsistent with the orbital ephemeris given by Galloway et al. (2005) unless a correction is made to the orbital epoch.

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