NASA NTRS · 20140012504
GBM Observations of Be X-Ray Binary Outbursts
Abstract
Since 2008 we have been monitoring accreting pulsars using the Gamma ray Burst Monitor (GBM) on Fermi. This monitoring program includes daily blind full sky searches for previously unknown or previously quiescent pulsars and source specific analysis to track the frequency evolution of all detected pulsars. To date we have detected outbursts from 23 transient accreting pulsars, including 21 confirmed or likely Be/X‐ray binaries. I will describe our techniques and highlight results for selected pulsars.
Keep this discovery
Explore connections, maps & timelines
Wilson-Hodge, Colleen A., Finger, M. H., Jenke, P. A.. 2014-07-07. GBM Observations of Be X-Ray Binary Outbursts. https://ntrs.nasa.gov/citations/20140012504
Cite the original work for its findings. Save a collection to share your selection of sources.