Absolute Magnitude Distribution And Light Curves Of Gamma-Ray Burst Supernovae

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Accepted by AJ, 16 pages, 5 figures

Scientific paper

10.1088/0004-6256/137/1/347

Photometry data were collected from the literature and analyzed for supernovae that are thought to have a gamma-ray burst association. There are several gamma-ray burst afterglow light curves that appear to have a supernova component. For these light curves, the supernova component was extracted and analyzed. A supernova light curve model was used to help determine the peak absolute magnitudes as well as estimates for the kinetic energy, ejected mass and nickel mass in the explosion. The peak absolute magnitudes are, on average, brighter than those of similar supernovae (stripped-envelope supernovae) that do not have a gamma-ray burst association, but this can easily be due to a selection effect. However, the kinetic energies and ejected masses were found to be considerably higher, on average, than those of similar supernovae without a gamma-ray burst association.

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

Absolute Magnitude Distribution And Light Curves Of Gamma-Ray Burst Supernovae 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 Absolute Magnitude Distribution And Light Curves Of Gamma-Ray Burst Supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Absolute Magnitude Distribution And Light Curves Of Gamma-Ray Burst Supernovae will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-528554

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