Deep searches for pulsations in SGR 1627-41 and 0526-66

Details Deep searches for pulsations in SGR 1627-41 and 0526-66 Deep searches for pulsations in SGR 1627-41 and 0526-66

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..526..786m&link_type=abstract

GAMMA-RAY BURSTS: 5th Huntsville Symposium. AIP Conference Proceedings, Volume 526, pp. 786-790 (2000).

Computer Science

X-Ray Sources, X-Ray Bursts, Pulsars, Neutron Stars

Scientific paper

Deep searches for X-ray pulsations from SGR 1627-41 and SGR 0526-66 were performed with ASCA. SGR 1806-20 and 1900+14 were previously established as X-ray pulsars. SGR 0526-66 is suspected to be a strong candidate for a magnetar, but X-ray pulsation has not been confirmed yet. Detection of X-ray pulsations from SGR 1627-41 and SGR 0526-66, is the key issue to the unified magnetar model of the SGRs. Although ASCA has done the deepest observations of ~80 ks for both of them, we did not detect pulsations. The long-term period history of SGR 1900+14 is compared with a very similar change of the AXP pulsar 1E1048.1-5937. .

Affiliated with

Also associated with

No associations

Rating

Deep searches for pulsations in SGR 1627-41 and 0526-66 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 Deep searches for pulsations in SGR 1627-41 and 0526-66, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Deep searches for pulsations in SGR 1627-41 and 0526-66 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1523441