NAOC Open IR
SN 2016X: a type II-P supernova with a signature of shock breakout from explosion of a massive red supergiant
Huang, F.1,2,3,4; Wang, X. -F.1,2; Hosseinzadeh, G.5,6; Brown, P. J.7; Mo, J.1,2; Zhang, J. -J.4,8,9; Zhang, K. -C.1,2; Zhang, T. -M.10; Howell, D. -A.5,6; Arcavi, I.5,6; McCully, C.5,6; Valenti, S.11; Rui, L. -M.1,2; Song, H.1,2; Xiang, D. -F.1,2; Li, W. -X.1,2; Lin, H.1,2; Wang, L. -F.7
2018-04-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume475Issue:3Pages:3959-3973
AbstractWe present extensive ultraviolet (UV) and optical photometry, as well as dense optical spectroscopy, for type II Plateau (1IP) supernova SN 2016X that exploded in the nearby (similar to 15 Mpc) spiral galaxy UGC 08041. The observations span the period from 2 to 180 d after the explosion; in particular, the Swift UV data probably captured the signature of shock breakout associated with the explosion of SN 2016X. It shows very strong UV emission during the first week after explosion, with a contribution of similar to 20-30 per cent to the bolometric luminosity (versus less than or similar to 15 per cent for normal SNe IIP). Moreover, we found that this supernova has an unusually long rise time of about 12.6 +/- 0.5 d in the R band (versus similar to 7.0 d for typical SNe IIP). The optical light curves and spectral evolution are quite similar to the fast-declining type IIP object SN 2013ej, except that SN 2016X has a relatively brighter tail. Based on the evolution of photospheric temperature as inferred from the Swift data in the early phase, we derive that the progenitor of SN 2016X has a radius of about 930 +/- 70 R-circle dot This large-size star is expected to be a red supergiant star with an initial mass of greater than or similar to 19-20 M-circle dot based on the mass-radius relation of the Galactic red supergiants, and it represents one of the most largest and massive progenitors found for SNe IIP.
Keywordsupernovae: general supernovae: individual: SN 2016X galaxies: individual: UGC 08041
Funding OrganizationChinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; US NSF ; US NSF ; NASA through the Einstein Fellowship Program ; NASA through the Einstein Fellowship Program ; NASA's Astrophysics Data Analysis Program ; NASA's Astrophysics Data Analysis Program ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; US NSF ; US NSF ; NASA through the Einstein Fellowship Program ; NASA through the Einstein Fellowship Program ; NASA's Astrophysics Data Analysis Program ; NASA's Astrophysics Data Analysis Program ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; US NSF ; US NSF ; NASA through the Einstein Fellowship Program ; NASA through the Einstein Fellowship Program ; NASA's Astrophysics Data Analysis Program ; NASA's Astrophysics Data Analysis Program ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; US NSF ; US NSF ; NASA through the Einstein Fellowship Program ; NASA through the Einstein Fellowship Program ; NASA's Astrophysics Data Analysis Program ; NASA's Astrophysics Data Analysis Program ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program
DOI10.1093/mnras/sty066
WOS KeywordCORE-COLLAPSE SUPERNOVAE ; LIGHT CURVES ; X-RAY ; PHYSICAL-PROPERTIES ; PLATEAU SUPERNOVAE ; PROGENITOR ; SWIFT ; TELESCOPE ; EVOLUTION ; 2005CS
Language英语
Funding ProjectChinese Academy of Sciences ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC)[11178003] ; National Natural Science Foundation of China (NSFC)[11325313] ; National Natural Science Foundation of China (NSFC)[11633002] ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences[OP201702] ; US NSF[1313484] ; NASA through the Einstein Fellowship Program[PF6-170148] ; NASA's Astrophysics Data Analysis Program[NNX13AF35G] ; NSFC[11403096] ; NSFC[11773067] ; NSFC[11203034] ; Key Research Program of the CAS[KJZD-EW-M06] ; Youth Innovation Promotion Association of the CAS ; CAS 'Light of West China' Program
Funding OrganizationChinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; US NSF ; US NSF ; NASA through the Einstein Fellowship Program ; NASA through the Einstein Fellowship Program ; NASA's Astrophysics Data Analysis Program ; NASA's Astrophysics Data Analysis Program ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; US NSF ; US NSF ; NASA through the Einstein Fellowship Program ; NASA through the Einstein Fellowship Program ; NASA's Astrophysics Data Analysis Program ; NASA's Astrophysics Data Analysis Program ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; US NSF ; US NSF ; NASA through the Einstein Fellowship Program ; NASA through the Einstein Fellowship Program ; NASA's Astrophysics Data Analysis Program ; NASA's Astrophysics Data Analysis Program ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Collaborating Research Program of the Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; US NSF ; US NSF ; NASA through the Einstein Fellowship Program ; NASA through the Einstein Fellowship Program ; NASA's Astrophysics Data Analysis Program ; NASA's Astrophysics Data Analysis Program ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000427141900074
PublisherOXFORD UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/37074
Collection中国科学院国家天文台
Corresponding AuthorHuang, F.
Affiliation1.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
2.Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China
3.Shanghai Jiao Tong Univ, Dept Astron, Shanghai 200240, Peoples R China
4.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Yunnan, Peoples R China
5.Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
6.Las Cumbres Observ, 6740 Cortona Dr Suite 102, Goleta, CA 93117 USA
7.Texas A&M Univ, Dept Phys & Astron, George P & Cynthia Woods Mitchell Inst Fundamenta, 4242 TAMU, College Stn, TX 77843 USA
8.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China
9.Chinese Acad Sci, Ctr Astron Mega Sci, 20A Datun Rd, Beijing 100012, Peoples R China
10.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100012, Peoples R China
11.Univ Calif Davis, Dept Phys, 1 Shields Ave, Davis, CA 95616 USA
Recommended Citation
GB/T 7714
Huang, F.,Wang, X. -F.,Hosseinzadeh, G.,et al. SN 2016X: a type II-P supernova with a signature of shock breakout from explosion of a massive red supergiant[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,475(3):3959-3973.
APA Huang, F..,Wang, X. -F..,Hosseinzadeh, G..,Brown, P. J..,Mo, J..,...&Wang, L. -F..(2018).SN 2016X: a type II-P supernova with a signature of shock breakout from explosion of a massive red supergiant.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,475(3),3959-3973.
MLA Huang, F.,et al."SN 2016X: a type II-P supernova with a signature of shock breakout from explosion of a massive red supergiant".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 475.3(2018):3959-3973.
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