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![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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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 |
DOI | 10.1051/0004-6361/202244985 |
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. |
入库方式: OAI收割
来源:新疆天文台
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