Accreting Pulsars Detected with Fermi GBM

Details Accreting Pulsars Detected with Fermi GBM Accreting Pulsars Detected with Fermi GBM

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.1008f&link_type=abstract

American Astronomical Society, HEAD meeting #11, #10.08; Bulletin of the American Astronomical Society, Vol. 41, p.670

Astronomy and Astrophysics

Astronomy

Scientific paper

Cen X-3 is a luminous accreting pulsar in an eclipsing binary system. From the precise obit determinations which have been made over the past 40 years we know that the orbital period is decreasing. The pulsar's spin frequency history shows torque switching behavior with rapid transitions between intervals of fairly constant spin-up and fairly constant spin-down. We present Fermi Gamma-ray Burst Monitor (GBM) observations of Cen X-3, from which we re-determine the orbital parameters. We also present an analysis of the torque behavior based on these observations.

Affiliated with

Also associated with

No associations

Rating

Accreting Pulsars Detected with Fermi GBM does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Accreting Pulsars Detected with Fermi GBM, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Accreting Pulsars Detected with Fermi GBM will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1092429