The long-lived Type IIn SN 2015da: Infrared echoes and strong interaction within an extended massive shell star star star
文献类型：期刊论文
| 作者 | Tartaglia, L.2,3; Pastorello, A.4; Sollerman, J.2,3; Fransson, C.2,3; Mattila, S.5; Fraser, M.6; Taddia, F.2,3; Tomasella, L.4; Turatto, M.4; Morales-Garoffolo, A.7 |
| 刊名 | ASTRONOMY & ASTROPHYSICS
 |
| 出版日期 | 2020-03-04 |
| 卷号 | 635页码:22 |
| 关键词 | supernovae: general galaxies: individual: NGC 5337 supernovae: individual: PSN J13522411+3941286 supernovae: individual: iPTF16tu supernovae: individual: SN 2015da |
| ISSN号 | 0004-6361 |
| DOI | 10.1051/0004-6361/201936553 |
| 英文摘要 | In this paper we report the results of the first similar to four years of spectroscopic and photometric monitoring of the Type IIn supernova SN 2015da (also known as PSN J13522411+3941286, or iPTF16tu). The supernova exploded in the nearby spiral galaxy NGC 5337 in a relatively highly extinguished environment. The transient showed prominent narrow Balmer lines in emission at all times and a slow rise to maximum in all bands. In addition, early observations performed by amateur astronomers give a very well-constrained explosion epoch. The observables are consistent with continuous interaction between the supernova ejecta and a dense and extended H-rich circumstellar medium. The presence of such an extended and dense medium is difficult to reconcile with standard stellar evolution models, since the metallicity at the position of SN 2015da seems to be slightly subsolar. Interaction is likely the mechanism powering the light curve, as confirmed by the analysis of the pseudo bolometric light curve, which gives a total radiated energy greater than or similar to 10(51) erg. Modeling the light curve in the context of a supernova shock breakout through a dense circumstellar medium allowed us to infer the mass of the prexisting gas to be similar or equal to 8 M-circle dot, with an extreme mass-loss rate for the progenitor star similar or equal to 0.6 M-circle dot yr(-1), suggesting that most of the circumstellar gas was produced during multiple eruptive events. Near- and mid-infrared observations reveal a fluxexcess in these domains, similar to those observed in SN 2010jl and other interacting transients, likely due to preexisting radiatively heated dust surrounding the supernova. By modeling the infrared excess, we infer a mass greater than or similar to 0.4 x 10(-3) M-circle dot for the dust. |
| WOS关键词 | RICH CIRCUMSTELLAR MEDIUM ; IA SUPERNOVA ; LUMINOUS SUPERNOVA ; ETA-CARINAE ; STELLAR EVOLUTION ; EMISSION-LINES ; SHOCK BREAKOUT ; LIGHT-CURVE ; H-I ; DUST |
| 资助项目 | Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Royal Society -Science Foundation Ireland University Research Fellowship ; Finnish Cultural Foundation ; Vilho, Yrjo and Kalle Vaisala Foundation of the Finnish Academy of Science and Letters ; NSF[AST-1821987] ; NSF[AST-1821967] ; NSF[AST-1813708] ; NSF[AST-1813466] ; NSF[AST-1908972] ; NSF[AST-1313484] ; NSF[AST-1813176] ; PRIN-INAF 2016 with the project "Towards the SKA and CTA era: discovery, localisation, and physics of transient sources" ; Spanish MICINN grant[ESP2017-82674-R] ; FEDER funds ; National Natural Science Foundation of China (NSFC grants)[11325313] ; National Natural Science Foundation of China (NSFC grants)[11633002] ; National Natural Science Foundation of China (NSFC grants)[11761141001] ; National Natural Science Foundation of China (NSFC grants)[11773067] ; National Natural Science Foundation of China (NSFC grants)[11403096] ; National Program on Key Research and Development Project[2016YFA0400803] ; Youth Innovation Promotion Association of the CAS[2018081] ; Western Light Youth Project ; Gemini Observatory[GN2016B-Q-57] ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Science Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy ; Japanese Monbukagakusho ; Max Planck Society ; University of Chicago ; Fermilab ; Institute for Advanced Study ; Japan Participation Group ; Johns Hopkins University ; Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; University of Pittsburgh ; Princeton University ; United States Naval Observatory ; University of Washington |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000519108600001 |
| 出版者 | EDP SCIENCES S A |
| 资助机构 | Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Royal Society -Science Foundation Ireland University Research Fellowship ; Royal Society -Science Foundation Ireland University Research Fellowship ; Finnish Cultural Foundation ; Finnish Cultural Foundation ; Vilho, Yrjo and Kalle Vaisala Foundation of the Finnish Academy of Science and Letters ; Vilho, Yrjo and Kalle Vaisala Foundation of the Finnish Academy of Science and Letters ; NSF ; NSF ; PRIN-INAF 2016 with the project "Towards the SKA and CTA era: discovery, localisation, and physics of transient sources" ; PRIN-INAF 2016 with the project "Towards the SKA and CTA era: discovery, localisation, and physics of transient sources" ; Spanish MICINN grant ; Spanish MICINN grant ; FEDER funds ; FEDER funds ; National Natural Science Foundation of China (NSFC grants) ; National Natural Science Foundation of China (NSFC grants) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; Western Light Youth Project ; Western Light Youth Project ; Gemini Observatory ; Gemini Observatory ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; University of Chicago ; University of Chicago ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Royal Society -Science Foundation Ireland University Research Fellowship ; Royal Society -Science Foundation Ireland University Research Fellowship ; Finnish Cultural Foundation ; Finnish Cultural Foundation ; Vilho, Yrjo and Kalle Vaisala Foundation of the Finnish Academy of Science and Letters ; Vilho, Yrjo and Kalle Vaisala Foundation of the Finnish Academy of Science and Letters ; NSF ; NSF ; PRIN-INAF 2016 with the project "Towards the SKA and CTA era: discovery, localisation, and physics of transient sources" ; PRIN-INAF 2016 with the project "Towards the SKA and CTA era: discovery, localisation, and physics of transient sources" ; Spanish MICINN grant ; Spanish MICINN grant ; FEDER funds ; FEDER funds ; National Natural Science Foundation of China (NSFC grants) ; National Natural Science Foundation of China (NSFC grants) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; Western Light Youth Project ; Western Light Youth Project ; Gemini Observatory ; Gemini Observatory ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; University of Chicago ; University of Chicago ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Royal Society -Science Foundation Ireland University Research Fellowship ; Royal Society -Science Foundation Ireland University Research Fellowship ; Finnish Cultural Foundation ; Finnish Cultural Foundation ; Vilho, Yrjo and Kalle Vaisala Foundation of the Finnish Academy of Science and Letters ; Vilho, Yrjo and Kalle Vaisala Foundation of the Finnish Academy of Science and Letters ; NSF ; NSF ; PRIN-INAF 2016 with the project "Towards the SKA and CTA era: discovery, localisation, and physics of transient sources" ; PRIN-INAF 2016 with the project "Towards the SKA and CTA era: discovery, localisation, and physics of transient sources" ; Spanish MICINN grant ; Spanish MICINN grant ; FEDER funds ; FEDER funds ; National Natural Science Foundation of China (NSFC grants) ; National Natural Science Foundation of China (NSFC grants) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; Western Light Youth Project ; Western Light Youth Project ; Gemini Observatory ; Gemini Observatory ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; University of Chicago ; University of Chicago ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Royal Society -Science Foundation Ireland University Research Fellowship ; Royal Society -Science Foundation Ireland University Research Fellowship ; Finnish Cultural Foundation ; Finnish Cultural Foundation ; Vilho, Yrjo and Kalle Vaisala Foundation of the Finnish Academy of Science and Letters ; Vilho, Yrjo and Kalle Vaisala Foundation of the Finnish Academy of Science and Letters ; NSF ; NSF ; PRIN-INAF 2016 with the project "Towards the SKA and CTA era: discovery, localisation, and physics of transient sources" ; PRIN-INAF 2016 with the project "Towards the SKA and CTA era: discovery, localisation, and physics of transient sources" ; Spanish MICINN grant ; Spanish MICINN grant ; FEDER funds ; FEDER funds ; National Natural Science Foundation of China (NSFC grants) ; National Natural Science Foundation of China (NSFC grants) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; Western Light Youth Project ; Western Light Youth Project ; Gemini Observatory ; Gemini Observatory ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; University of Chicago ; University of Chicago ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/56418]  |
| 专题 | 中国科学院国家天文台 |
| 通讯作者 | Tartaglia, L. |
| 作者单位 | 1.Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA 2.Stockholm Univ, AlbaNova, Dept Astron, Roslagstullsbacken 21, S-11421 Stockholm, Sweden 3.Stockholm Univ, AlbaNova, Oskar Klein Ctr, Roslagstullsbacken 21, S-11421 Stockholm, Sweden 4.Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy 5.Univ Turku, Dept Phys & Astron, Tuorla Observ, Turku 20014, Finland 6.Univ Coll Dublin, Sch Phys, OBrien Ctr Sci North, Belfield Dublin 4, Ireland 7.Univ Cadiz, Dept Appl Phys, Campus Puerto Real, Cadiz 11510, Spain 8.CSIC, Inst Space Sci ICE, Campus UAB,Cami Can Magrans S-N, Barcelona 08193, Spain 9.IEEC, C Gran Capita 2-4,Edif Nexus 201, Barcelona 08034, Spain 10.Weizmann Inst Sci, Benoziyo Ctr Astrophys, IL-76100 Rehovot, Israel |
| 推荐引用方式 GB/T 7714 | Tartaglia, L.,Pastorello, A.,Sollerman, J.,et al. The long-lived Type IIn SN 2015da: Infrared echoes and strong interaction within an extended massive shell star star star[J]. ASTRONOMY & ASTROPHYSICS,2020,635:22. |
| APA | Tartaglia, L..,Pastorello, A..,Sollerman, J..,Fransson, C..,Mattila, S..,...&Terreran, G..(2020).The long-lived Type IIn SN 2015da: Infrared echoes and strong interaction within an extended massive shell star star star.ASTRONOMY & ASTROPHYSICS,635,22. |
| MLA | Tartaglia, L.,et al."The long-lived Type IIn SN 2015da: Infrared echoes and strong interaction within an extended massive shell star star star".ASTRONOMY & ASTROPHYSICS 635(2020):22. |
入库方式： OAI收割
来源：国家天文台
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