An Interpretation of the $hν_{peak}$ - $E_{iso}$ Correlation for GRB

Details An Interpretation of the $hν_{peak}$ - $E_{iso}$ Correlation for GRB An Interpretation of the $hν_{peak}$ - $E_{iso}$ Correlation for GRB

2004-05-03

arxiv.org/abs/astro-ph/0405014v1

Astrophys.J. 614 (2004) L13-L16

Astronomy and Astrophysics

Astrophysics

12 pages. 5 figures

Scientific paper

10.1086/425310

The $h\nu_{peak}/100 KeV \sim [E_{iso}/10^{52} \rm{erg}]^{1/2}$ correlation
reported recently by Amati et al. (2002) and Lamb et al. (2003) for long GRB's
can be interpreted as a viewing angle effect if the emitting region of the
fireball is ring-shaped.

Affiliated with

Also associated with

No associations

Rating

An Interpretation of the $hν_{peak}$ - $E_{iso}$ Correlation for GRB 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 An Interpretation of the $hν_{peak}$ - $E_{iso}$ Correlation for GRB, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An Interpretation of the $hν_{peak}$ - $E_{iso}$ Correlation for GRB will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-234595