SN 2021wuf: A transitional type Ia supernova with a low-velocity gradient
文献类型:期刊论文
作者 | Zeng, Xiangyun7,8; Li, Sai6,7,8; Wang, Xiaofeng3,6,15; Zheng, Sheng7,8; Andrew Howell, D.2,14; Azaleee Bostroem, K.2,14; Mccully, Curtis14,15; Esamdin, Ali4![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
![]() |
出版日期 | 2024-10-31 |
卷号 | 691页码:A90 |
关键词 | supernovae: individual: SN 2021wuf |
ISSN号 | 0004-6361 |
DOI | 10.1051/0004-6361/202451048 |
产权排序 | 7 |
英文摘要 | In this paper, we present an extensive analysis of SN 2021 wuf, a transition between Ia-norm and SN 1991T-like supernovae, which exploded at the periphery of the tidal bridge between the pair galaxy NGC 6500 and NGC 6501, at a redshift of z = 0.01. Our observations, ranging from -21 to +276 days relative to the B-band maximum light, reveal that SN 2021wuf exhibits properties akin to normal SNe Ia, with a peak absolute magnitude of M-max(B) similar to - 19.49 +/- 0.10 mag and a post-peak decline rate of Delta m(15)(B) similar to 1.11 +/- 0.06 mag. The peak bolometric luminosity of this SN is estimated as 1.58 x 10(43) erg s(-1), corresponding to a Ni-56 mass of M-Ni similar to 0.64 +/- 0.05 M-circle dot. The spectral features, including high-velocity Si II lambda 6355 lines, a plateau in the Si II lambda 6355 velocity evolution and the nickel-to-iron ratio in the nebular phase, suggest a potential pulsating delayed detonation mechanism. The absence of intermediate-mass elements in the early phase and the high photospheric temperature, as inferred from the line-strength ratio of Si II lambda 5972 to Si II lambda 6355 (named as R(Si II)), further support this classification. |
WOS关键词 | WHITE-DWARF MODELS ; LATE-TIME SPECTRA ; LIGHT CURVES ; SPECTROSCOPIC OBSERVATIONS ; CIRCUMSTELLAR MATERIAL ; OPTICAL OBSERVATIONS ; FACTORY OBSERVATIONS ; PROGENITOR SYSTEM ; EXPLOSION ; ULTRAVIOLET |
资助项目 | National Natural Science Foundation of China ; National Key R&D program of China for Intergovernmental Scientific and TechnologicalInnovation Cooperation Project[2022YFE0126200] ; High Level Talent-Heaven Lake Program of Xinjiang Uygur Autonomous Region of China ; Tencent Xplorer prize ; NSF[AST-1911225] ; NSF[AST-1911151] ; NASA[NN12AR55G] ; NASA[80NSSC18K0284] ; NASA[80NSSC18K1575] ; Asteroid Terrestrial-impact Last Alert System (ATLAS) project ; Asteroid Terrestrial-impact Last Alert System (ATLAS) ; Queen's University Belfast ; South African Astronomical Observatory ; [12288102] ; [12033003] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:001346445300003 |
出版者 | EDP SCIENCES S A |
资助机构 | National Natural Science Foundation of China ; National Key R&D program of China for Intergovernmental Scientific and TechnologicalInnovation Cooperation Project ; High Level Talent-Heaven Lake Program of Xinjiang Uygur Autonomous Region of China ; Tencent Xplorer prize ; NSF ; NASA ; Asteroid Terrestrial-impact Last Alert System (ATLAS) project ; Asteroid Terrestrial-impact Last Alert System (ATLAS) ; Queen's University Belfast ; South African Astronomical Observatory |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/7117] ![]() |
专题 | 光学天文与技术应用研究室_变星研究团组 新疆天文台_光学天文与技术应用研究室 |
通讯作者 | Wang, Xiaofeng; Zheng, Sheng |
作者单位 | 1.Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamental, Dept Phys & Astron, 4242 TAMU, College Stn, TX 77843 USA 2.Las Cumbres Observ, 6740 Cortona Dr,Suite 102, Goleta, CA 93117 USA 3.Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China 4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 5.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China 6.Beijing Acad Sci & Technol, Beijing Planetarium, Beijing 100044, Peoples R China 7.China Three Gorges Univ, Coll Sci, Yichang 443000, Peoples R China 8.China Three Gorges Univ, Ctr Astron & Space Sci, Yichang 443000, Peoples R China 9.Chinese Acad Sci, Yunnan Observ YNAO, Kunming 650216, Peoples R China 10.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650216, Peoples R China |
推荐引用方式 GB/T 7714 | Zeng, Xiangyun,Li, Sai,Wang, Xiaofeng,et al. SN 2021wuf: A transitional type Ia supernova with a low-velocity gradient[J]. ASTRONOMY & ASTROPHYSICS,2024,691:A90. |
APA | Zeng, Xiangyun.,Li, Sai.,Wang, Xiaofeng.,Zheng, Sheng.,Andrew Howell, D..,...&Zhang, Junjie.(2024).SN 2021wuf: A transitional type Ia supernova with a low-velocity gradient.ASTRONOMY & ASTROPHYSICS,691,A90. |
MLA | Zeng, Xiangyun,et al."SN 2021wuf: A transitional type Ia supernova with a low-velocity gradient".ASTRONOMY & ASTROPHYSICS 691(2024):A90. |
入库方式: OAI收割
来源:新疆天文台
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。