NAOC Open IR
How are gamma-ray burst radio afterglows populated?
Zhang, K.1,3; Zhang, Z. B.1; Huang, Y. F.2; Song, L. M.3; Zheng, S. J.3; Li, X. J.1; Li, D.4,5; Su, F. F.1
2021-05-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume503Issue:3Pages:3262-3278
AbstractWe systematically analyse two GRB samples with radio-loud and radio-quiet afterglows, respectively. It is interestingly found that the radio-selected GRB samples exhibit a clear dichotomy in terms of their distributions of intrinsic durations (T-int), isotropic energies in gamma-rays (E-gamma,E- iso), the circum-burst medium density (n), the spectral radio peak luminosity (L-nu,L- p) and flux densities (F-host) of host galaxies. On average, the values of T-int, E-gamma,E- iso, n, L-nu,L- p, and F-host of radio-quiet GRBs are relatively smaller than those of radio-loud ones. However, the redshifts and host flux densities of both samples are similarly distributed. In addition, a positive power-law correlation of L-nu,L- p proportional to E-gamma,iso(0.41 +/- 0.04) is found for the radio-loud sample, especially in accord with the supernova-associated GRBs, which is marginally consistent with that of the radio-quiet GRB sample. A negative correlation between T-int and z is confirmed to similarly hold for both radio-loud and radio-quiet GRBs. The dividing line between short and long GRBs in the rest frame is at T-int similar or equal to 1 s. Consequently, we propose that the radio-selected GRBs could be originated from distinct progenitors and central engines, together with environments.
Keywordmethods: data analysis galaxies: general radio continuum: ISM radio continuum: transients gamma-ray bursts transients: supernovae
Funding OrganizationMinistry of Science and Technology of the People's Republic of China ; Ministry of Science and Technology of the People's Republic of China ; Research Foundation of China ; Research Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Ministry of Science and Technology of the People's Republic of China ; Ministry of Science and Technology of the People's Republic of China ; Research Foundation of China ; Research Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Ministry of Science and Technology of the People's Republic of China ; Ministry of Science and Technology of the People's Republic of China ; Research Foundation of China ; Research Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Ministry of Science and Technology of the People's Republic of China ; Ministry of Science and Technology of the People's Republic of China ; Research Foundation of China ; Research Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; National Key Research and Development Program of China ; National Key Research and Development Program of China
DOI10.1093/mnras/stab465
WOS KeywordBROAD-BAND AFTERGLOW ; HUBBLE DIAGRAM ; LIGHT-CURVE ; BLACK-HOLE ; GRB 970508 ; REDSHIFT ; STAR ; ENERGETICS ; DURATION ; MERGER
Language英语
Funding ProjectMinistry of Science and Technology of the People's Republic of China[2020SKA0120300] ; Research Foundation of China[ZR2018MA030] ; Research Foundation of China[XKJJC201901] ; Research Foundation of China[201909118] ; National Natural Science Foundation of China[U2031118] ; National Natural Science Foundation of China[11988101] ; National Natural Science Foundation of China[12041306] ; National Natural Science Foundation of China[U1938201] ; National Natural Science Foundation of China[11873030] ; National Natural Science Foundation of China[11673023] ; National Natural Science Foundation of China[U1838201] ; National Natural Science Foundation of China[U1838202] ; National Natural Science Foundation of China[U1838104] ; National Natural Science Foundation of China[11725313] ; National Natural Science Foundation of China[11690024] ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe')[XDB23040000] ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe')[XDA15360300] ; National Key Research and Development Program of China[2016YFA0400800] ; National Key Research and Development Program of China[2017YFA0402600]
Funding OrganizationMinistry of Science and Technology of the People's Republic of China ; Ministry of Science and Technology of the People's Republic of China ; Research Foundation of China ; Research Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Ministry of Science and Technology of the People's Republic of China ; Ministry of Science and Technology of the People's Republic of China ; Research Foundation of China ; Research Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Ministry of Science and Technology of the People's Republic of China ; Ministry of Science and Technology of the People's Republic of China ; Research Foundation of China ; Research Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; Ministry of Science and Technology of the People's Republic of China ; Ministry of Science and Technology of the People's Republic of China ; Research Foundation of China ; Research Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; Strategic Priority Research Program of the Chinese Academy of Sciences ('Multiwaveband Gravitational Wave Universe') ; National Key Research and Development Program of China ; National Key Research and Development Program of China
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000649000600010
PublisherOXFORD UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/77816
Collection中国科学院国家天文台
Corresponding AuthorZhang, Z. B.; Huang, Y. F.; Li, D.
Affiliation1.Qufu Normal Univ, Coll Phys & Engn, Qufu 273165, Shandong, Peoples R China
2.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China
3.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
4.Chinese Acad Sci, Natl Astron Observ China, 20A Datun Rd, Beijing 100020, Peoples R China
5.Univ KwaZulu Natal, NAOC UKZN Computat Astrophys Ctr, ZA-4000 Durban, South Africa
Recommended Citation
GB/T 7714
Zhang, K.,Zhang, Z. B.,Huang, Y. F.,et al. How are gamma-ray burst radio afterglows populated?[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2021,503(3):3262-3278.
APA Zhang, K..,Zhang, Z. B..,Huang, Y. F..,Song, L. M..,Zheng, S. J..,...&Su, F. F..(2021).How are gamma-ray burst radio afterglows populated?.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,503(3),3262-3278.
MLA Zhang, K.,et al."How are gamma-ray burst radio afterglows populated?".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 503.3(2021):3262-3278.
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