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A Monte Carlo Approach to Magnetar-powered Transients. II. Broad-lined Type Ic Supernovae Not Associated with GRBs
Wang, L. J.1,2; Cano, Z.3; Wang, S. Q.4,5,6; Zheng, W. K.6; Liu, L. D.4,5; Deng, J. S.2; Yu, H.4,5; Dai, Z. G.4,5; Han, Y. H.2; Xu, D.2; Qiu, Y. L.2; Wei, J. Y.2; Li, B.1,4; Song, L. M.1
2017-12-10
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume851Issue:1Pages:16
AbstractBroad-lined type Ic supernovae (SNe Ic-BL) are a subclass of rare core-collapse SNe whose energy source is debated in the literature. Recently, a series of investigations on SNe Ic-BL with the magnetar (plus Ni-56) model were carried out. Evidence for magnetar formation was found for the well-observed SNe Ic-BL 1998bw and 2002ap. In this paper, we systematically study a large sample of SNe Ic-BL not associated with gamma-ray bursts (GRBs). We use photospheric velocity data determined in a homogeneous way. We find that the magnetar+ Ni-56 model provides a good description of the light curves and velocity evolution of our sample of SNe Ic-BL, although some SNe (not all) can also be described by the pure-magnetar model or by the two-component pure-Ni-56 model (three out of 12 are unlikely to be explained by two-component model). In the magnetar+ Ni-56 model, the amount of Ni-56 required to explain their luminosity is significantly reduced, and the derived initial explosion energy is, in general, in accordance with neutrino heating. Some correlations between different physical parameters are evaluated, and their implications regarding magnetic field amplification and the total energy reservoir are discussed.
Keywordstars: neutron supernovae: general
Funding OrganizationNational Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; National Basic Research Program of China ("973" Program) ; National Basic Research Program of China ("973" Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; National Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; National Basic Research Program of China ("973" Program) ; National Basic Research Program of China ("973" Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; National Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; National Basic Research Program of China ("973" Program) ; National Basic Research Program of China ("973" Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; National Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; National Basic Research Program of China ("973" Program) ; National Basic Research Program of China ("973" Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS
DOI10.3847/1538-4357/aa9a38
WOS KeywordCORE-COLLAPSE SUPERNOVAE ; GAMMA-RAY BURST ; LIGHT CURVES ; SUPERLUMINOUS SUPERNOVAE ; SN 1998BW ; HYPERNOVA ; EXTINCTION ; DIVERSITY ; EVOLUTION ; EMISSION
Language英语
Funding ProjectNational Program on Key Research and Development Project of China[2016YFA0400801] ; National Basic Research Program of China ("973" Program)[2014CB845800] ; National Natural Science Foundation of China[U1331202] ; National Natural Science Foundation of China[11533033] ; National Natural Science Foundation of China[U1331101] ; National Natural Science Foundation of China[11673006] ; National Natural Science Foundation of China[11573014] ; National Natural Science Foundation of China[11422325] ; National Natural Science Foundation of China[11373022] ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS[XDB23040100]
Funding OrganizationNational Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; National Basic Research Program of China ("973" Program) ; National Basic Research Program of China ("973" Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; National Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; National Basic Research Program of China ("973" Program) ; National Basic Research Program of China ("973" Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; National Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; National Basic Research Program of China ("973" Program) ; National Basic Research Program of China ("973" Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; National Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; National Basic Research Program of China ("973" Program) ; National Basic Research Program of China ("973" Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; One-Hundred-Talent Program from the National Astronomical Observatories, Chinese Academy of Sciences) ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS ; Strategic Priority Research Program "Multi-wavelength Gravitational Wave Universe" of the CAS
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000417907200003
PublisherIOP PUBLISHING LTD
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/37345
Collection中国科学院国家天文台
Corresponding AuthorWang, L. J.
Affiliation1.Chinese Acad Sci, Inst High Energy Phys, Astroparticle Phys, Beijing 100049, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Key Lab Space Astron & Technol, Beijing 100012, Peoples R China
3.CSIC, IAA, Glorieta Astron S-N, E-18008 Granada, Spain
4.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
5.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Jiangsu, Peoples R China
6.Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
Recommended Citation
GB/T 7714
Wang, L. J.,Cano, Z.,Wang, S. Q.,et al. A Monte Carlo Approach to Magnetar-powered Transients. II. Broad-lined Type Ic Supernovae Not Associated with GRBs[J]. ASTROPHYSICAL JOURNAL,2017,851(1):16.
APA Wang, L. J..,Cano, Z..,Wang, S. Q..,Zheng, W. K..,Liu, L. D..,...&Song, L. M..(2017).A Monte Carlo Approach to Magnetar-powered Transients. II. Broad-lined Type Ic Supernovae Not Associated with GRBs.ASTROPHYSICAL JOURNAL,851(1),16.
MLA Wang, L. J.,et al."A Monte Carlo Approach to Magnetar-powered Transients. II. Broad-lined Type Ic Supernovae Not Associated with GRBs".ASTROPHYSICAL JOURNAL 851.1(2017):16.
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