中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A comparative analysis of type Ia supernovae 2018xx and 2019gbx

文献类型:期刊论文

作者Li, Yangyang15,16; Zheng, Sheng15,16; Zeng, Xiangyun15,16; Wang, Xiaofeng12,13,14; Burke, Jamison10,11; Pellegrino, Craig10,11; Esamdin, Ali9; Lin, Xinkui9; Wang, Yong9; Iskandar, Abdusamatjan8,9
刊名ASTRONOMY & ASTROPHYSICS
出版日期2023-07-03
卷号675页码:15
关键词supernovae: general supernovae: individual: SN 2018xx supernovae: individual: SN 2019gbx
ISSN号0004-6361
DOI10.1051/0004-6361/202244985
通讯作者Zeng, Xiangyun(xyzeng2018@ctgu.edu.cn) ; Wang, Xiaofeng(wang_xf@mail.tsinghua.edu.cn)
英文摘要We present a comparative study of two nearby type Ia supernovae (SNe Ia), 2018xx and 2019gbx, that exploded in NGC 4767 and MCG-02-33-017 at a distance of 48 Mpc and 60 Mpc, respectively. The B-band light curve decline rate for SN 2018xx is estimated to be 1.48 & PLUSMN; 0.07 mag and for SN 2019gbx it is 1.37 & PLUSMN; 0.07 mag. Despite the similarities in photometric evolution, quasi-bolometric luminosity, and spectroscopy between these two SNe Ia, SN 2018xx has been found to be fainter by about & SIM;0.38 mag in the B-band and has a lower Ni-56 yield. Their host galaxies have similar metallicities at the SN location, indicating that the differences between these two SNe Ia may be associated with the higher progenitor metallicity of SN 2018xx. Further inspection of the near-maximum-light spectra has revealed that SN 2018xx has relatively strong absorption features near 4300 & ANGS; relative to SN 2019gbx. The application of the code TARDIS fitting to the above features indicates that the absorption features near 4300 & ANGS; appear to be related to not only Fe II/Mg II abundance but possibly to the other element abundances as well. Moreover, SN 2018xx shows a weaker carbon absorption at earlier times, which is also consistent with higher ejecta metallicity.
WOS关键词SPECTRAL ENERGY-DISTRIBUTION ; TIME OPTICAL-SPECTRA ; HOST GALAXIES ; LIGHT CURVES ; SN 2011FE ; IMPROVED DISTANCES ; RISE-TIME ; LUMINOSITY ; METALLICITY ; MODEL
资助项目National Natural Science Foundation of China[12033003] ; National Natural Science Foundation of China[11633002] ; High Level Talent-Heaven Lake Program of Xinjiang Uygur Autonomous Region of China ; Scholar Program of Beijing Academy of Science and Technology[80NSSC19K1639] ; Tencent Xplorer prize ; NSF[U2031202] ; NSF[12203029] ; NASA[12288102] ; National Natural Science Foundation of China (NSFC) ; [DZ:BS202002] ; [AST-1911225] ; [AST-1911151]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001022371200010
出版者EDP SCIENCES S A
资助机构National Natural Science Foundation of China ; High Level Talent-Heaven Lake Program of Xinjiang Uygur Autonomous Region of China ; Scholar Program of Beijing Academy of Science and Technology ; Tencent Xplorer prize ; NSF ; NASA ; National Natural Science Foundation of China (NSFC)
源URL[http://ir.xao.ac.cn/handle/45760611-7/5380]  
专题研究单元未命名
通讯作者Zeng, Xiangyun; Wang, Xiaofeng
作者单位1.Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, Dept Phys & Astron, 4242 TAMU, College Stn, TX 77843 USA
2.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China
3.Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel
4.Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
5.Chinese Acad Sci, Ctr Astron Mega Sci, 20A Datun Rd, Beijing, Peoples R China
6.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650216, Peoples R China
7.Chinese Acad Sci, Yunnan Observ YNAO, Kunming 650216, Peoples R China
8.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
9.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
10.Las Cumbres Observ, 6740 Cortona Dr Suite 102, Goleta, CA 93117 USA
推荐引用方式
GB/T 7714
Li, Yangyang,Zheng, Sheng,Zeng, Xiangyun,et al. A comparative analysis of type Ia supernovae 2018xx and 2019gbx[J]. ASTRONOMY & ASTROPHYSICS,2023,675:15.
APA Li, Yangyang.,Zheng, Sheng.,Zeng, Xiangyun.,Wang, Xiaofeng.,Burke, Jamison.,...&Zhou, Guangrong.(2023).A comparative analysis of type Ia supernovae 2018xx and 2019gbx.ASTRONOMY & ASTROPHYSICS,675,15.
MLA Li, Yangyang,et al."A comparative analysis of type Ia supernovae 2018xx and 2019gbx".ASTRONOMY & ASTROPHYSICS 675(2023):15.

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