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ATel #11780; P. Jenke (UAH-SPA/CSPAR), C. A. Wilson-Hodge (NASA/MSFC), C. Malacaria (NASA/MSFC-USRA), O. Roberts (USRA) on 25 Jun 2018; 19:45 UTCredential Certification: Peter Jenke (peter.a.jenke@nasa.gov)
Subjects: X-ray, Gamma Ray, Binary, Neutron Star, Transient, Pulsar
Referred to by ATel #: 11791
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Fermi/GBM is detecting renewed activity from the Be X-ray binary Cep X-4 (Ginga 2138+56). Pulsations at 15.0703(8) mHz with a pulsed flux of 9.2 +/- 0.5 mCrab (12-25 keV) were observed on 20 June. The last outburst occurred on 06 June 2014.
GBM Accreting Pulsar Histories
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