Constraints on the Diverse Progenitors of GRBs from the Large-Scale Environments

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Invited review to appear in the Proceedings of the 16th Annual October Astrophysics Conference in Maryland, "Gamma Ray Bursts

Scientific paper

10.1063/1.2207943

The pursuit of the progenitors of short duration-hard spectrum gamma-ray bursts (SHBs) draws strongly upon similar quests for the origin of supernovae (SNe) and long duration-soft spectrum GRBs(LSBs). Indeed the notion that, in the absence of smoking guns, the progenitors of cosmic explosions betray their identities both on the global and local scale, motivates the study of SHB redshifts, host galaxies, and locations with respect to hosts. To this end, we suggest both a historical and emergent physical analogy of GRBs with SNe: long-soft GRBs are to core-collapsed supernovae as short-hard GRBs are to Type Ia supernovae ("LSB:CC::SHB:Ia''). Still, the SHB progenitor pursuit is just beginning and we caution that while there are some substantive differences between observations of LSBs and SHBs on large-scales, particularly in host demographics, neither the offset nor the redshift distributions of SHBs are statistically inconsistent with those of LSBs.

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

Constraints on the Diverse Progenitors of GRBs from the Large-Scale Environments 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 Constraints on the Diverse Progenitors of GRBs from the Large-Scale Environments, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Constraints on the Diverse Progenitors of GRBs from the Large-Scale Environments will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-484196

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