伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章,另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.

星期二, 九月 14, 2010

Goldstein 2010 伽马暴的一种新的分类方法:E_P/Fluence

主要内容:


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灰色的是“短暴“


文章信息:

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Title:
A New Discriminator for Gamma-ray Burst Classification: The E peak-fluence Energy Ratio
Authors:
Goldstein, Adam; Preece, Robert D.; Briggs, Michael S.
Affiliation:
AA(Physics Department, The University of Alabama in Huntsville, Huntsville, AL 35809, USA), AB(Physics Department, The University of Alabama in Huntsville, Huntsville, AL 35809, USA), AC(Physics Department, The University of Alabama in Huntsville, Huntsville, AL 35809, USA)
Publication:
The Astrophysical Journal, Volume 721, Issue 2, pp. 1329-1332 (2010). (ApJ Homepage)
Publication Date:
10/2010
Origin:
IOP
ApJ Keywords:
gamma-ray burst: general, methods: data analysis
DOI:
10.1088/0004-637X/721/2/1329
Bibliographic Code:
2010ApJ...721.1329G

Abstract

Using the derived gamma-ray burst (GRB) E peak and fluences from the complete BATSE 5B Spectral Catalog, we study the ensemble characteristics of the E peak-fluence relation for GRBs. This relation appears to be a physically meaningful and insightful fundamental discriminator between long and short bursts. We discuss the results of the lower limit test of the E peak-E iso relations in the E peak-fluence plane for Burst And Transient Source Experiment bursts with no observed redshift. Our results confirm the presence of two GRB classes as well as heavily suggesting two different GRB progenitor types.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)

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