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Title: Possible Correlations between the Emission Properties of SGRBs and Their Offsets from the Host Galaxies

Abstract

Short gamma-ray bursts (SGRBs) are widely believed to be from mergers of binary compact objects involving at least one neutron star and hence have a broad range of spatial offsets from their host galaxies. In this work, we search for possible correlations between the emission properties of 18 SGRBs and their offsets from the host galaxies. The SGRBs with and without extended emission do not show significant differences between their offset distributions, in agreement with some previous works. There are, however, possible correlations between the optical and X-ray afterglow emission and the offsets. The underlying physical origins are examined.

Authors:
; ; ; ;  [1];  [2]
  1. Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210008 (China)
  2. College of Science, Guilin University of Technology, Guilin 541004 (China)
Publication Date:
OSTI Identifier:
22663356
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal; Journal Volume: 844; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; AFTERGLOW; CORRELATIONS; COSMIC GAMMA BURSTS; DISTRIBUTION; EMISSION; GALAXIES; GAMMA RADIATION; NEUTRON STARS; NEUTRONS; X RADIATION

Citation Formats

Zhang, Shuai, Jin, Zhi-Ping, Li, Xiang, Fan, Yi-Zhong, Wei, Da-Ming, and Zhang, Fu-Wen, E-mail: jin@pmo.ac.cn, E-mail: yzfan@pmo.ac.cn, E-mail: dmwei@pmo.ac.cn. Possible Correlations between the Emission Properties of SGRBs and Their Offsets from the Host Galaxies. United States: N. p., 2017. Web. doi:10.3847/1538-4357/AA7AA7.
Zhang, Shuai, Jin, Zhi-Ping, Li, Xiang, Fan, Yi-Zhong, Wei, Da-Ming, & Zhang, Fu-Wen, E-mail: jin@pmo.ac.cn, E-mail: yzfan@pmo.ac.cn, E-mail: dmwei@pmo.ac.cn. Possible Correlations between the Emission Properties of SGRBs and Their Offsets from the Host Galaxies. United States. doi:10.3847/1538-4357/AA7AA7.
Zhang, Shuai, Jin, Zhi-Ping, Li, Xiang, Fan, Yi-Zhong, Wei, Da-Ming, and Zhang, Fu-Wen, E-mail: jin@pmo.ac.cn, E-mail: yzfan@pmo.ac.cn, E-mail: dmwei@pmo.ac.cn. Thu . "Possible Correlations between the Emission Properties of SGRBs and Their Offsets from the Host Galaxies". United States. doi:10.3847/1538-4357/AA7AA7.
@article{osti_22663356,
title = {Possible Correlations between the Emission Properties of SGRBs and Their Offsets from the Host Galaxies},
author = {Zhang, Shuai and Jin, Zhi-Ping and Li, Xiang and Fan, Yi-Zhong and Wei, Da-Ming and Zhang, Fu-Wen, E-mail: jin@pmo.ac.cn, E-mail: yzfan@pmo.ac.cn, E-mail: dmwei@pmo.ac.cn},
abstractNote = {Short gamma-ray bursts (SGRBs) are widely believed to be from mergers of binary compact objects involving at least one neutron star and hence have a broad range of spatial offsets from their host galaxies. In this work, we search for possible correlations between the emission properties of 18 SGRBs and their offsets from the host galaxies. The SGRBs with and without extended emission do not show significant differences between their offset distributions, in agreement with some previous works. There are, however, possible correlations between the optical and X-ray afterglow emission and the offsets. The underlying physical origins are examined.},
doi = {10.3847/1538-4357/AA7AA7},
journal = {Astrophysical Journal},
number = 1,
volume = 844,
place = {United States},
year = {Thu Jul 20 00:00:00 EDT 2017},
month = {Thu Jul 20 00:00:00 EDT 2017}
}
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