Still Brighter than Pre-explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart
文献类型:期刊论文
作者 | McCully, Curtis13,14; Jha, Saurabh W.15; Scalzo, Richard A.4,16; Howell, D. Andrew13,14; Foley, Ryan J.5; Ceng YT(曾耀田)6,7,8; Liu ZW(柳正伟)6,7,9; Hosseinzadeh, Griffin10; Bildsten, Lars11,14; Riess, Adam G.1,12 |
刊名 | ASTROPHYSICAL JOURNAL |
出版日期 | 2022-02-01 |
卷号 | 925期号:2 |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/ac3bbd |
产权排序 | 第7完成单位 |
文献子类 | Article |
英文摘要 | Type Iax supernovae (SNe Iax) represent the largest class of peculiar white dwarf supernovae. The type Iax SN 2012Z in NGC 1309 is the only white dwarf supernova with a detected progenitor system in pre-explosion observations. Deep Hubble Space Telescope (HST) images taken before SN 2012Z show a luminous, blue source that we have interpreted as a helium-star companion (donor) to the exploding white dwarf. We present here late-time HST observations taken similar to 1400 days after the explosion to test this model. We find the SN light curve can empirically be fit by an exponential-decay model in magnitude units. The fitted asymptotic brightness is within 10% of our latest measurements and approximately twice the brightness of the pre-explosion source. The decline of the light curve is too slow to be powered by Co-56 or Co-57 decay: if radioactive decay is the dominate power source, it must be from longer half-life species like Fe-55. Interaction with circumstellar material may contribute to the light curve, as may shock heating of the companion star. Companion-star models underpredict the observed flux in the optical, producing most of their flux in the UV at these epochs. A radioactively heated bound remnant, left after only a partial disruption of the white dwarf, is also capable of producing the observed excess late-time flux. Our analysis suggests that the total ejecta + remnant mass is consistent with the Chandrasekhar mass for a range of SNe Iax. |
学科主题 | 天文学 ; 恒星与银河系 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | LATE-TIME SPECTROSCOPY ; IAX SUPERNOVA ; WHITE-DWARF ; PROGENITOR SYSTEMS ; LIGHT-CURVE ; FAINT TYPE ; HELIUM ; CONSTRAINTS ; EVOLUTION ; 2005HK |
资助项目 | NSFNational Science Foundation (NSF)[AST-1518052] ; NSFNational Science Foundation (NSF)[AST-1313484] ; NSFNational Science Foundation (NSF)[AST-1615455] ; NASA HST programs[HST-GO-12913] ; NASA HST programs[HST-GO-13360] ; NASA HST programs[HST-GO-13757] ; Gordon & Betty Moore FoundationGordon and Betty Moore Foundation ; Heising-Simons Foundation ; David and Lucile Packard FoundationThe David & Lucile Packard Foundation ; National Natural Science Foundation of China (NSFC)National Natural Science Foundation of China (NSFC)[11873016] ; Chinese Academy of Sciences, and Yunnan Province[202001AW070007] ; NASANational Aeronautics & Space Administration (NASA)[HST-GO-12913] ; NASANational Aeronautics & Space Administration (NASA)[HST-GO-13360] ; NASANational Aeronautics & Space Administration (NASA)[HST-GO-13757] ; NASANational Aeronautics & Space Administration (NASA)[NAS5-26555] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP Publishing Ltd |
WOS记录号 | WOS:000749298700001 |
资助机构 | NSFNational Science Foundation (NSF)[AST-1518052, AST-1313484, AST-1615455] ; NASA HST programs[HST-GO-12913, HST-GO-13360, HST-GO-13757] ; Gordon & Betty Moore FoundationGordon and Betty Moore Foundation ; Heising-Simons Foundation ; David and Lucile Packard FoundationThe David & Lucile Packard Foundation ; National Natural Science Foundation of China (NSFC)National Natural Science Foundation of China (NSFC)[11873016] ; Chinese Academy of Sciences, and Yunnan Province[202001AW070007] ; NASANational Aeronautics & Space Administration (NASA)[HST-GO-12913, HST-GO-13360, HST-GO-13757, NAS5-26555] |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/24853] |
专题 | 云南天文台_大样本恒星演化研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
通讯作者 | McCully, Curtis |
作者单位 | 1.Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, USA; 2.Gordon and Betty Moore Foundation, 1661 Page Mill Road, Palo Alto, CA 94304, USA; 3.University of Texas at Austin, 1 University Station C1400, Austin, TX 78712-0259, USA 4.Centre for Translational Data Science, University of Sydney, Darlington, NSW 2008, Australia; 5.Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 92064, USA; 6.Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming 650216, People's Republic of China; 7.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming 650216, People's Republic of China; 8.University of Chinese Academy of Science, Beijing 100012, People's Republic of China; 9.Center for Astronomical Mega-Science, CAS, Beijing 100012, People's Republic of China; 10.Center for Astrophysics ∣ Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138-1516, USA; |
推荐引用方式 GB/T 7714 | McCully, Curtis,Jha, Saurabh W.,Scalzo, Richard A.,et al. Still Brighter than Pre-explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart[J]. ASTROPHYSICAL JOURNAL,2022,925(2). |
APA | McCully, Curtis.,Jha, Saurabh W..,Scalzo, Richard A..,Howell, D. Andrew.,Foley, Ryan J..,...&Camacho-Neves, Yssavo.(2022).Still Brighter than Pre-explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart.ASTROPHYSICAL JOURNAL,925(2). |
MLA | McCully, Curtis,et al."Still Brighter than Pre-explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart".ASTROPHYSICAL JOURNAL 925.2(2022). |
入库方式: OAI收割
来源:云南天文台
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