Publication Date:
2019-07-19
Description:
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/Xray binaries. I will describe our techniques and highlight results for selected pulsars.
Keywords:
Astronomy
Type:
M14-3642
,
Be X-Ray Binary Systems (BeXRB) 2014 Worksbop; Jul 07, 2014 - Jul 11, 2014; Valencia; Spain
Format:
application/pdf