Too Observations of Soft Gamma Repeaters

Details Too Observations of Soft Gamma Repeaters Too Observations of Soft Gamma Repeaters

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1212w&link_type=abstract

Chandra Proposal ID #04500502

Physics

Chandra Proposal Id #04500502

Scientific paper

Soft Gamma Repeaters are rare sources of transient burst emission, probably magnetars (i.e. strongly magnetized neutron stars). Each of the SGRs has a persistent X-ray counterpart and some show coherent pulsations. During burst active phases, these counterparts undergo changes in their energy spectrum and pulse properties. Measuring the effects of burst activity are diagnostic of the burst mechanism and their nature in general. In the event of detection of substantial burst activity from an SGR, we propose to make Chandra ToO observations of any of the four known sources, SGR 1900+14, SGR 1806-20, SGR 1627-41, SGR 0526-66, the SGR candidate SGR 1801-23, as well as any newly discovered SGR source.

Affiliated with

Also associated with

No associations

Rating

Too Observations of Soft Gamma Repeaters 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 Too Observations of Soft Gamma Repeaters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Too Observations of Soft Gamma Repeaters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1042439