A Two-Component Explosion Model for the Giant Flare and Radio Afterglow from SGR 1806-20-Reference-Cited by-同舟云学术

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A Two-Component Explosion Model for the Giant Flare and Radio Afterglow from SGR 1806-20

Published:2005-08-02 Issue:2 Volume:629 Page:L81-L84
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Dai Z. G.,Wu X. F.,Wang X. Y.,Huang Y. F.,Zhang B.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference33 articles.

1. Detection of a radio counterpart to the 27 December 2004 giant flare from SGR 1806–20

2. Cea, P. 2005, preprint (astro-ph/0504020)

3. The Radio Afterglow from the Giant Flare of SGR 1900+14: The Same Mechanism as Afterglows from Classic Gamma-Ray Bursts?

4. The connection between W31, SGR 1806–20, and LBV 1806–20: Distance, extinction, and structure

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2. Magnetar giant flare originating from GRB 200415A: transient GeV emission, time-resolved Ep – L iso correlation and implications;Research in Astronomy and Astrophysics;2021-11-01

3. Radio afterglow rebrightening: evidence for multiple active phases in gamma-ray burst central engines;Astrophysics and Space Science;2015-08-29

4. Radio afterglows and host galaxies of gamma-ray bursts;Monthly Notices of the Royal Astronomical Society;2015-06-09

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