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Gamma-ray bursts subset and supernova remnants low radio-frequency turnover
Liu, X
2000
Source PublicationCHINESE PHYSICS LETTERS
ISSN0256-307X
Volume17Issue:8Pages:623-624
Contribution Rank1
Abstract

Durations of gamma-ray bursts (GRB's) are featured by >2 s subset and <2 s one, with initial corresponding energy ratio being 20:1. It is found that supernova remants(SNR's) turnover frequencies peak at 100 and 500 MHz. After assuming that GRB's originate from hypernova and making an analysis on the evolution of GRB's, we find that the initial energy of two GRB subsets leads to a different radio-frequency turnover of their remnant spectra, which accords positively with the turnover-frequency ratio of SNR's.

KeywordAfterglow Discovery
SubtypeArticle
Subject Area星系和宇宙学
WOS HeadingsScience & Technology ; Physical Sciences
Indexed BySCI
Language英语
WOS KeywordAfterglow ; Discovery
Funding Project星系宇宙学研究团组
WOS Research AreaPhysics
WOS SubjectPhysics, Multidisciplinary
WOS IDWOS:000088961900029
Funding Organization95 Key Project of Basic Research of Chinese Academy of Sciences (Grant No.KJ952-J303)
Citation statistics
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/159
Collection射电天文研究室_星系宇宙学研究团组
射电天文研究室
Corresponding AuthorLiu, X
AffiliationChinese Acad Sci, Natl Astron Observ, Urumqi Astron Observ, Urumqi 830011, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Liu, X. Gamma-ray bursts subset and supernova remnants low radio-frequency turnover[J]. CHINESE PHYSICS LETTERS,2000,17(8):623-624.
APA Liu, X.(2000).Gamma-ray bursts subset and supernova remnants low radio-frequency turnover.CHINESE PHYSICS LETTERS,17(8),623-624.
MLA Liu, X."Gamma-ray bursts subset and supernova remnants low radio-frequency turnover".CHINESE PHYSICS LETTERS 17.8(2000):623-624.
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