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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; Wang, X. -F.1; Hosseinzadeh, G.4,5; Brown, P. J.6; Mo, J.1; Zhang JJ(张居甲)3,7,8; Zhang, K. -C.1; Zhang, T. -M.9; Howell, D. -A.4,5; Arcavi, I.4,5; McCully, C.4,5; Valenti, S.10; Rui, L. -M.1; Song, H.1; Xiang, D. -F.1; Li, W. -X.1; Lin, H.1; Wang, L. -F.6; Huang, F.(Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China)
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2018-04-01
卷号475期号:3页码:3959-3973
DOI10.1093/mnras/sty066
产权排序第7完成单位
收录类别SCI
关键词Supernovae: General Supernovae: Individual: Sn 2016x Galaxies: Individual: Ugc 08041
摘要We 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.
项目资助者Chinese Academy of Sciences ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC)(11178003, 11325313, 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, 11773067, 11203034) ; Key Research Program of the CAS(KJZD-EW-M06) ; Youth Innovation Promotion Association of the CAS ; CAS 'Light of West China' Program
语种英语
学科领域天文学
文章类型Article
ISSN0035-8711
URL查看原文
WOS记录号WOS:000427141900074
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]CORE-COLLAPSE SUPERNOVAE ; LIGHT CURVES ; X-RAY ; PHYSICAL-PROPERTIES ; PLATEAU SUPERNOVAE ; PROGENITOR ; SWIFT ; TELESCOPE ; EVOLUTION ; 2005CS
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被引频次:2[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/12299
专题丽江天文观测站(南方基地)
中国科学院天体结构与演化重点实验室
通讯作者Huang, F.(Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China)
作者单位1.Physics Department and Tsinghua Centre for Astrophysics, Tsinghua University, Beijing 100084, China
2.Department of Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China
3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
4.Department of Physics, University of California, Santa Barbara, CA 93106-9530, USA
5.Las Cumbres Observatory, 6740 Cortona Dr, Suite 102, Goleta, CA 93117-5575, USA
6.Department of Physics and Astronomy, George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station, TX 77843, USA
7.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
8.Centre for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China
9.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
10.Department of Physics, University of California, 1 Shields Avenue, Davis, CA 95616-5270, USA
11.Univ Calif Davis, Dept Phys, 1 Shields Ave, Davis, CA 95616 USA
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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..,...&Huang, 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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