Thompson 2010 磁星作为伽马暴的能源机制

主要内容:


精彩摘抄:


文章信息:

· Find Similar Abstracts (with default settings below)

· arXiv e-print (arXiv:1008.5138)

· References in the Article

· Also-Read Articles (Reads History)

·

· Translate This Page

Title:		Proto-Magnetars as GRB Central Engines: Uncertainties, Limitations, and Particulars
Authors:		Thompson, Todd A.; Metzger, Brian D.; Bucciantini, Niccolò
Publication:		eprint arXiv:1008.5138
Publication Date:		08/2010
Origin:		ARXIV
Keywords:		Astrophysics - High Energy Astrophysical Phenomena
Comment:		8 pages. Proceedings for Deciphering the Ancient Universe with GRBs, Kyoto, Japan, April, 2010
Bibliographic Code:		2010arXiv1008.5138T

Abstract

The millisecond proto-magnetar model for the central engine of long-duration gamma-ray bursts is briefly reviewed. Limitations and uncertainties in the model are highlighted. A short discussion of the maximum energy, maximum duration, radiative efficiency, jet formation mechanism, late-time energy injection, and (non-)association with supernovae of millisecond magnetar-powered GRBs is provided.

---

Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)