NAOC Open IR
The optical properties of three Type II supernovae: 2014cx, 2014cy, and 2015cz
Dastidar, R.1,2; Misra, K.1; Singh, M.1,3; Pastorello, A.4; Sahu, D. K.5; Wang, X.6,7,8; Gangopadhyay, A.1,9; Tomasella, L.4; Zhang, J.10,11; Bose, S.12,13; Mo, J.6,7; Elias-Rosa, N.4,14; Tartaglia, L.15,16; Yan, S.6,7; Kumar, Brijesh1; Anupama, G. C.5; Pandey, S. B.1; Rui, L.6,7; Zhang, T.17; Terreran, G.18,19; Ochner, P.4; Huang, F.20
2021-06-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume504Issue:1Pages:1009-1028
AbstractWe present the photometric and spectroscopic analysis of three Type II supernovae (SNe): 2014cx, 2014cy, and 2015cz. SN 2014cx is a conventional Type IIP with shallow slope (0.2 mag/50 d) and an atypical short plateau (similar to 86 d). SNe 2014cy and 2015cz show relatively large decline rates (0.88 and 1.64 mag/50 d, respectively) at early times before settling to the plateau phase, unlike the canonical Type IIP/L SN light curves. All of them are normal luminosity SN II with an absolute magnitude at mid-plateau of M-V,14cx(50) = -16.6 +/- 0.4 mag, M-V,14cy(50) = -16.5 +/- 0.2 mag, and M-V,15cz(50) = -17.4 +/- 0.3 mag. A relatively broad range of Ni-56 masses is ejected in these explosions (0.027-0.070M(circle dot)). The spectra shows the classical evolution of SNe II, dominated by a blue continuum with broad H lines at early phases and narrower metal lines with PCygni profiles during the plateau. High-velocity H I features are identified in the plateau spectra of SN 2014cx at 11 600 kms(-1), possibly a sign of ejecta-circumstellar interaction. The spectra of SN 2014cy exhibit strong absorption profile of HI similar to normal luminosity events whereas strong metal lines akin to sub-luminous SNe. The analytical modelling of the bolometric light curve of the three events yields similar progenitor radii within errors (478, 507, and 660 R-circle dot for SNe 2014cx, 2014cy, and 2015cz, respectively), a range of ejecta masses (15.0, 22.2, and 20.6M(circle dot) for SNe 2014cx, 2014cy, and 2015cz), and a modest range of explosion energies (3.3-7.2 foe where 1 foe=10(51) erg).
Keywordtechniques: photometric techniques: spectroscopic supernovae: general supernovae: individual: SN 2014cx, SN 2014cy, SN 2015cz galaxies: individual: NGC 337, NGC 7742, NGC 582
Funding OrganizationNational Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; DST/JSPS (Japan Society for the Promotion of Science) ; DST/JSPS (Japan Society for the Promotion of Science) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; DST/JSPS (Japan Society for the Promotion of Science) ; DST/JSPS (Japan Society for the Promotion of Science) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; DST/JSPS (Japan Society for the Promotion of Science) ; DST/JSPS (Japan Society for the Promotion of Science) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; DST/JSPS (Japan Society for the Promotion of Science) ; DST/JSPS (Japan Society for the Promotion of Science)
DOI10.1093/mnras/stab831
WOS KeywordLIGHT-CURVES ; PHYSICAL-PROPERTIES ; SN 1999EM ; METALLICITY ; ABUNDANCES ; GALAXIES ; DISTANCE ; MODEL
Language英语
Funding ProjectNational Aeronautics and Space Administration ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC)[11325313] ; National Natural Science Foundation of China (NSFC)[11633002] ; National Natural Science Foundation of China (NSFC)[11761141001] ; National Program on Key Research and Development Project[2016YFA0400803] ; BRICS (Brazil, Russia, India, China, and South Africa) grant[DST/IMRCD/BRICS/Pilotcall/ProFCheap/2017(G)] ; DST/JSPS (Japan Society for the Promotion of Science)[DST/INT/JSPS/P/281/2018]
Funding OrganizationNational Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; DST/JSPS (Japan Society for the Promotion of Science) ; DST/JSPS (Japan Society for the Promotion of Science) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; DST/JSPS (Japan Society for the Promotion of Science) ; DST/JSPS (Japan Society for the Promotion of Science) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; DST/JSPS (Japan Society for the Promotion of Science) ; DST/JSPS (Japan Society for the Promotion of Science) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; BRICS (Brazil, Russia, India, China, and South Africa) grant ; DST/JSPS (Japan Society for the Promotion of Science) ; DST/JSPS (Japan Society for the Promotion of Science)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000656137100073
PublisherOXFORD UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/77447
Collection中国科学院国家天文台
Corresponding AuthorDastidar, R.
Affiliation1.Aryabhatta Res Inst Observat Sci, Naini Tal 263001, India
2.Univ Delhi, Dept Phys & Astrophys, Delhi 110007, India
3.Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea
4.INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy
5.Indian Inst Astrophys, Bangalore 560034, Karnataka, India
6.Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China
7.Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China
8.Beijing Acad Sci & Technol, Beijing Planetarium, Beijing 100044, Peoples R China
9.Pt Ravi Shankar Shukla Univ, Raipur 492010, Madhya Pradesh, India
10.Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China
11.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650216, Yunnan, Peoples R China
12.Ohio State Univ, Dept Astron, 140 W 18th Ave, Columbus, OH 43210 USA
13.Ohio State Univ, Ctr Cosmol & AstroParticle Phys CCAPP, 191 W Woodruff Ave, Columbus, OH 43210 USA
14.CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, E-08193 Barcelona, Spain
15.Stockholm Univ, AlbaNova Univ Ctr, Dept Astron, SE-10691 Stockholm, Sweden
16.Stockholm Univ, AlbaNova Univ Ctr, Oskar Klein Ctr, SE-10691 Stockholm, Sweden
17.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China
18.Northwestern Univ, Ctr Interdisciplinary Explorat & Res Astrophys CI, Evanston, IL 60208 USA
19.Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA
20.Shanghai Jiao Tong Univ, Dept Astron, Shanghai 200240, Peoples R China
Recommended Citation
GB/T 7714
Dastidar, R.,Misra, K.,Singh, M.,et al. The optical properties of three Type II supernovae: 2014cx, 2014cy, and 2015cz[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2021,504(1):1009-1028.
APA Dastidar, R..,Misra, K..,Singh, M..,Pastorello, A..,Sahu, D. K..,...&Huang, F..(2021).The optical properties of three Type II supernovae: 2014cx, 2014cy, and 2015cz.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,504(1),1009-1028.
MLA Dastidar, R.,et al."The optical properties of three Type II supernovae: 2014cx, 2014cy, and 2015cz".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 504.1(2021):1009-1028.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Dastidar, R.]'s Articles
[Misra, K.]'s Articles
[Singh, M.]'s Articles
Baidu academic
Similar articles in Baidu academic
[Dastidar, R.]'s Articles
[Misra, K.]'s Articles
[Singh, M.]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Dastidar, R.]'s Articles
[Misra, K.]'s Articles
[Singh, M.]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.