SN 2020pvb: A Type IIn-P supernova with a precursor outburst

doi:10.1051/0004-6361/202348790

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	SN 2020pvb: A Type IIn-P supernova with a precursor outburst
	Elias-Rosa, N.1,2; Brennan, S. J.3,4; Benetti, S.1; Cappellaro, E.1; Pastorello, A.1; Kozyreva, A.5; Lundqvist, P.3; Fraser, M.4; Anderson, J. P.6,7; Cai YZ(蔡永志)8,9,10 ; Chen, T.-W.11; Dennefeld, M.12; Gromadzki, M.13; Gutiérrez, C. P.2,14; Ihanec, N.13; Inserra, C.15; Kankare, E.16,17; Kotak, R.16; Mattila, S.16,18; Moran, S.16; Bravo, T. E.2,14; Pessi, P. J.3; Pignata, G.19; Reguitti, A.1,20; Reynolds, T. M.16,21; Smartt, S. J.22,23; Smith, K.23; Tartaglia, L.24; Valerin, G.1; De Boer, T.25; Chambers, K.25; Gal-Yam, A.26; Gao, H.25; Geier, S.27,28; Mazzali, P. A.29,30; Nicholl, M.23; Ragosta, F.31,32; Rest, A.33,34; Yaron, O.26; Young, D. R.23
发表期刊	Astronomy and Astrophysics
	2024-06-01
卷号	686
DOI	10.1051/0004-6361/202348790
产权排序	第8完成单位
收录类别	EI
关键词	supernovae: general supernovae: individual: SN 2020pvb
摘要	We present photometric and spectroscopic datasets for SN 2020pvb, a Type IIn-P supernova (SN) that is similar to SNe 1994W, 2005cl, 2009kn, and 2011ht, with a precursor outburst detected (PS1 w band ∼- 13.8 mag) around four months before the B-band maximum light. SN 2020pvb presents a relatively bright light curve that peaked at MB = -17.95 ± 0.30 mag and a plateau that lasted at least 40 days before going into solar conjunction. After this, the object was no longer visible at phases > 150 days above - 12.5 mag in the B band, suggesting that the SN 2020pvb ejecta interact with a dense, spatially confined circumstellar envelope. SN 2020pvb shows strong Balmer lines and a forest of Fe II lines with narrow P Cygni profiles in its spectra. Using archival images from the Hubble Space Telescope, we constrained the progenitor of SN 2020pvb to have a luminosity of log(L/Lo)≤5.4, ruling out any single star progenitor over 50 Mo. SN 2020pvb is a Type IIn-P whose progenitor star had an outburst*sim;0.5 yr before the final explosion; the material lost during this outburst probably plays a role in shaping the physical properties of the SN. © The Authors 2024.
资助项目	PRIN-INAF 2022; Science Foundation Ireland; Royal Society[101004719]; Royal Society - Science Foundation Ireland University Research Fellowship; EU Horizon 2020 research and innovation programme[2017/27/L/ST9/03221]; Polish NCN DAINA grant[350458]; Research Council of Finland[20215AT016]; Magnus Ehrnrooth Foundation; Spanish Ministerio de Ciencia e Innovacion (MCIN); Kalle Vaeisaelae Foundation; Agencia Estatal de Investigacion (AEI); Centro Superior de Investigaciones Cientificas (CSIC)[948381]; I-LINK 2021; Program Unidad de Excelencia Maria de Maeztu[ST/T000198/1]; European Research Council (ERC) under the European Union[ST/S006109/1]; Alan Turing Institute; Ministry of Economy, Development, and Tourism's Millennium Science Initiative[20179ZF5KS]; Millennium Institute of Astrophysics (MAS); Kalle Vaeisaelae Foundation of the Finnish academy of Science and Letters; STFC grant[12303054]; MIUR[ICN12_009]; National Natural Science Foundation of China (NSFC)[306531]; International Centre of Supernovae, Yunnan Key Laboratory[1103.D-0328]; Secretary of Universities and Research (Government of Catalonia); Horizon 2020 Research and Innovation Programme of the European Union under the Marie Sklodowska-Curie; Beatriu de Pinos; Spanish Ministerio de Ciencia e Innovacion (MCIN); ANID, Millennium Science Initiative[730890]; UK Science and Technology Facilities Council; Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias; STELLA robotic telescopes in Tenerife; Instrument Centre for Danish Astrophysics (IDA); Finnish Centre for Astronomy; ESO (FINCA); University of Turku, Finland[80NSSC18K0971]; European Southern Observatory under ESO programmes[NNX14AM74G]; European Southern Observatory under ESO programmes[NNX12AR65G]; European Union[80NSSC21K1572]; NASA SSO Near Earth Observation Program[ST/P000312/1]; NASA SSO Near Earth Observation Program[NN12AR55G]; NASA SSO Near Earth Observation Program[80NSSC18K0284]; NASA SSO Near Earth Observation Program[80NSSC18K1575]; NASA SSO Near Earth Observation Program[J1944/80NSSC19K0112]; NASA SSO Near Earth Observation Program[HST GO-15889]; State of Hawaii; STFC[12303054]; STFC[12540303]; STFC[202302AN360001]; NASA[PID2020-115253GA-I00]; NASA[LINKA20409]; NASA[BP00168]; Kepler/K2 grant; Heising-Simons Foundation;
项目资助者	PRIN-INAF 2022 ; Science Foundation Ireland ; Royal Society[101004719] ; Royal Society - Science Foundation Ireland University Research Fellowship ; EU Horizon 2020 research and innovation programme[2017/27/L/ST9/03221] ; Polish NCN DAINA grant[350458] ; Research Council of Finland[20215AT016] ; Magnus Ehrnrooth Foundation ; Spanish Ministerio de Ciencia e Innovacion (MCIN) ; Kalle Vaeisaelae Foundation ; Agencia Estatal de Investigacion (AEI) ; Centro Superior de Investigaciones Cientificas (CSIC)[948381] ; I-LINK 2021 ; Program Unidad de Excelencia Maria de Maeztu[ST/T000198/1] ; European Research Council (ERC) under the European Union[ST/S006109/1] ; Alan Turing Institute ; Ministry of Economy, Development, and Tourism's Millennium Science Initiative[20179ZF5KS] ; Millennium Institute of Astrophysics (MAS) ; Kalle Vaeisaelae Foundation of the Finnish academy of Science and Letters ; STFC grant[12303054] ; MIUR[ICN12_009] ; National Natural Science Foundation of China (NSFC)[306531] ; International Centre of Supernovae, Yunnan Key Laboratory[1103.D-0328] ; Secretary of Universities and Research (Government of Catalonia) ; Horizon 2020 Research and Innovation Programme of the European Union under the Marie Sklodowska-Curie ; Beatriu de Pinos ; Spanish Ministerio de Ciencia e Innovacion (MCIN) ; ANID, Millennium Science Initiative[730890] ; UK Science and Technology Facilities Council ; Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias ; STELLA robotic telescopes in Tenerife ; Instrument Centre for Danish Astrophysics (IDA) ; Finnish Centre for Astronomy ; ESO (FINCA) ; University of Turku, Finland[80NSSC18K0971] ; European Southern Observatory under ESO programmes[NNX14AM74G, NNX12AR65G] ; European Union[80NSSC21K1572] ; NASA SSO Near Earth Observation Program[ST/P000312/1, NN12AR55G, 80NSSC18K0284, 80NSSC18K1575, J1944/80NSSC19K0112, HST GO-15889] ; State of Hawaii ; STFC[12303054, 12540303, 202302AN360001] ; NASA[PID2020-115253GA-I00, LINKA20409, BP00168] ; Kepler/K2 grant ; Heising-Simons Foundation ; [RS-EA/3471] ; [CEX2020-001058-M] ; [IC120009] ; [106.216C] ; [NNX13AQ47G] ; [NNX08AR22G]
语种	英语
学科领域	天文学 ; 恒星与银河系
文章类型	Article
出版者	EDP SCIENCES S A
出版地	17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE
ISSN	0004-6361
URL	查看原文
WOS记录号	WOS:001230620000013
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	DIFFUSE INTERSTELLAR BANDS ; DIGITAL SKY SURVEY ; MASS-LOSS ; INTERACTING SUPERNOVAE ; PHYSICAL-PROPERTIES ; SPECTRAL EVOLUTION ; EXPLOSIVE EJECTION ; EMISSION-LINES ; LIGHT CURVES ; STAR
EI入藏号	20242216181029
EI主题词	Supernovae
EI分类号	657.2 Extraterrestrial Physics and Stellar Phenomena
引用统计
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/27352
专题	南方基地中国科学院天体结构与演化重点实验室
作者单位	1.INAF - Osservatorio Astronomico di Padova, vicolo dell'Osservatorio 5, Padova, 35122, Italy; 2.Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, Barcelona, 08193, Spain; 3.The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, Stockholm, 10691, Sweden; 4.School of Physics, O'Brien Centre for Science North, University College Dublin, Belfield, Dublin 4, Ireland; 5.Heidelberger Institut für Theoretische Studien, Schloss-Wolfsbrunnenweg 35, Heidelberg, 69118, Germany; 6.European Southern Observatory, Alonso de Córdova 3107 Casilla 19, Santiago, Chile; 7.Millennium Institute of Astrophysics (MAS), Nuncio Monseñor Sótero Sanz 100, Off. 104, Santiago, Chile; 8.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China; 9.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650216, China; 10.International Centre of Supernovae, Yunnan Key Laboratory, Kunming, 650216, China; 11.Graduate Institute of Astronomy, National Central University, 300 Jhongda Road, Jhongli, 32001, Taiwan; 12.CNRS, Institut d'Astrophysique de Paris (IAP), Sorbonne Université (Paris 6), 98bis, Boulevard Arago, Paris, 75014, France; 13.Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, Warszawa, 00-478, Poland; 14.Institut d'Estudis Espacials de Catalunya (IEEC), Barcelona, 08034, Spain; 15.Cardiff Hub for Astrophysics Research and Technology, School of Physics & Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, United Kingdom; 16.Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Turku, 20014, Finland; 17.Turku Collegium for Science, Medicine and Technology, University of Turku, Turku, 20014, Finland; 18.School of Sciences, European University Cyprus, Diogenes street, Engomi, Nicosia, 1516, Cyprus; 19.Instituto de Alta Investigación, Universidad de Tarapacá, Casilla 7D, Arica, Chile; 20.INAF, Osservatorio Astronomico di Brera, Via E. Bianchi 46, Merate, 23807, Italy; 21.Cosmic DAWN Centre, Niels Bohr Institute, University of Copenhagen, Jagtvej 128, København N, 2200, Denmark; 22.Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH, United Kingdom; 23.Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast, BT7 1NN, United Kingdom; 24.INAF - Osservatorio Astronomico d'Abruzzo, Via M. Maggini snc, Teramo, 64100, Italy; 25.Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI, 96822, United States; 26.Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, 76100, Israel; 27.Gran Telescopio Canarias (GRANTECAN), Cuesta de San José s/n, La Palma, 38712, Spain; 28.Instituto de Astrofísica de Canarias, Vía Láctea s/n, La Laguna, 38200, Spain; 29.Astrophysics Research Institute, Liverpool John Moores University, ic2, 146 Brownlow Hill, Liverpool, L3 5RF, United Kingdom; 30.Max-Planck Institut für Astrophysik, Karl-Schwarzschild-Str. 1, Garching bei München, 85741, Germany; 31.INAF, Osservatorio Astronomico di Roma, Via Frascati 33, Monte Porzio Catone (RM), 00078, Italy; 32.Space Science Data Center - ASI, Via del Politecnico SNC, Roma, 00133, Italy; 33.Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD, 21218, United States; 34.Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD, 21218, United States
推荐引用方式 GB/T 7714	Elias-Rosa, N.,Brennan, S. J.,Benetti, S.,et al. SN 2020pvb: A Type IIn-P supernova with a precursor outburst[J]. Astronomy and Astrophysics,2024,686.
APA	Elias-Rosa, N..,Brennan, S. J..,Benetti, S..,Cappellaro, E..,Pastorello, A..,...&Young, D. R..(2024).SN 2020pvb: A Type IIn-P supernova with a precursor outburst.Astronomy and Astrophysics,686.
MLA	Elias-Rosa, N.,et al."SN 2020pvb: A Type IIn-P supernova with a precursor outburst".Astronomy and Astrophysics 686(2024).

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