Detection of Orbital Period of EXO 1722-363

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

6

X-Ray, A Comment, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

In regards to Lutovinov et al.'s report of activity from EXO 1722-363 (ATEL #178), the source has been detected in RXTE PCA scans of the galactic center since Feb 1999. Ginga observations showed it to have a 413 s pulse period. (It was designated GPS 1722-363 by Tawara et al. 1989, PASJ, 41, 473.) Between Feb 1999 and 17 Aug 2003, the PCA scans measured a 2-10 keV flux range of 0-8 mCrab with random sampling of the pulse phase.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Detection of Orbital Period of EXO 1722-363 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 Detection of Orbital Period of EXO 1722-363, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of Orbital Period of EXO 1722-363 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1665091

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.