BeppoSAX observations of XRF 020427 and its afterglow

Details BeppoSAX observations of XRF 020427 and its afterglow BeppoSAX observations of XRF 020427 and its afterglow

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312..189a&link_type=abstract

Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference he

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We report preliminary results of the BeppoSAX measurements of the prompt and afterglow emission of XRF 020427, the second XRF for which X-ray afterglow emission was detected. We include in our analysis also the public data of the Chandra follow-up observations of this source. Our observations indicate that XRFs are characterized by the same afterglow emission properties of GRBs and favor the hypothesis that their extreme softness is due to inefficient shocks rather than a high off-axis viewing angle or a relatively high redshift.

Affiliated with

Also associated with

No associations

Rating

BeppoSAX observations of XRF 020427 and its afterglow 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 BeppoSAX observations of XRF 020427 and its afterglow, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and BeppoSAX observations of XRF 020427 and its afterglow will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-891001