Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-03-17
Astronomy and Astrophysics
Astrophysics
5 pages, 4 figures, submitted to ApJ Letters
Scientific paper
10.1086/312124
We report the discovery of a new soft gamma repeater (SGR), SGR 1627-41, and present BATSE observations of the burst emission and BeppoSAX NFI observations of the probable persistent X-ray counterpart to this SGR. All but one burst spectrum are well fit by an optically thin thermal bremsstrahlung (OTTB) model with kT values between 25 and 35 keV. The spectrum of the X-ray counterpart, SAX J1635.8-4736, is similar to that of other persistent SGR X-ray counterparts. We find weak evidence for a periodic signal at 6.41 s in the light curve for this source. Like other SGRs, this source appears to be associated with a young supernova remnant G337.0-0.1. Based upon the peak luminosities of bursts observed from this SGR, we find a lower limit on the dipole magnetic field of the neutron star B_dipole > 5 * 10^14 Gauss.
Briggs Michael Stephen
Dieters Stefan
Finger Mark H.
Fishman Gerald J.
Hurley Kevin
No associations
LandOfFree
Discovery of a New Soft Gamma Repeater, SGR 1627-41 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 Discovery of a New Soft Gamma Repeater, SGR 1627-41, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Discovery of a New Soft Gamma Repeater, SGR 1627-41 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-394534