Fireball/Blastwave Model and Soft γ-Ray Repeaters

Chin. Phys. Lett.

1998, Vol. 15

Issue (10): 775-777 DOI:

Original Articles

Fireball/Blastwave Model and Soft γ-Ray Repeaters

HUANG Yong-feng;DAI Zi-gao;LU Tan

Department of Astronomy, Nanjing University, Nanjing 210093

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HUANG Yong-feng, DAI Zi-gao, LU Tan 1998 Chin. Phys. Lett. 15 775-777

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Abstract Soft γ-ray repeaters are at determined distances and their positions are known accurately. If observed, afterglows from their soft γ-ray bursts will provide important clues to the study of the so called “classical γ-ray bursts”. On applying the popular fireball/blastwave model of classical γ-ray bursts to soft γ-ray repeaters, it is found that their x-ray and optical afterglows are detectable. Monitoring of the three repeaters is solicited.

Keywords: 98.20.Rz 98.70.Qy 97.60.Jd

Published: 01 October 1998

PACS:	98.20.Rz
	98.70.Qy	(X-ray sources; X-ray bursts)
	97.60.Jd	(Neutron stars)

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https://cpl.iphy.ac.cn/ OR https://cpl.iphy.ac.cn/Y1998/V15/I10/0775

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