New Outburst of the Be/X-ray Transient GRO J1750-27 Detected with Fermi/GBM
ATel #6839; Mark H. Finger (USRA) and Colleen A. Wilson-Hodge (NASA/MSFC) for the GBM Pulsar Project
on 19 Dec 2014; 22:40 UT
Distributed as an Instant Email Notice Transients
Credential Certification: Dr. Mark H. Finger (mark.h.finger@nasa.gov)
Subjects: X-ray, Binary, Neutron Star, Transient, Pulsar
Referred to by ATel #: 7096
Pulsations with a period near 4.45 s, consistent with GRO J1750-27, have been
detected with the 12-50 keV band of the GBM NaI detectors since December 13. The
orbitally corrected pulse frequency in the interval of December 16.0-19.0 was
224.6179(2) mHz.
The last outburst of this source was in 2008.
GBM Pulsar Project
