A GRB Model Satisfying Stringent Observational Constraints

Details A GRB Model Satisfying Stringent Observational Constraints A GRB Model Satisfying Stringent Observational Constraints

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.231..445s&link_type=abstract

Astrophysics and Space Science, Volume 231, Issue 1-2, pp. 445-448

Astronomy and Astrophysics

Astrophysics

3

Gamma Rays, Bursts

Scientific paper

The temporal behavior of GRBs is quantified using a power spectrum analysis. The power spectrum of great variety of GRBs is well represented by the simple ˜ω -2 behavior. We then study a cosmological GRB model in which relativistic flows interact with dense radiation fields. This mechanism in the densest stellar regions known to exist, surprisingly yields the correct temporal behavior. Other characteristics are also reproduced, including the duration bimodality and the hardness-duration distribution.

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