KMS of Xinjiang Astronomical Observatory, CAS
| A comparative analysis of type Ia supernovae 2018xx and 2019gbx | |
Li, Yangyang1,2; Zheng, Sheng1,2; Zeng, Xiangyun1,2; Wang, Xiaofeng3,4,5; Burke, Jamison6,7; Pellegrino, Craig6,7; Esamdin, Ali8 ; Lin, Xinkui8; Wang, Yong8; Iskandar, Abdusamatjan8,9; Zhang, Jujia10,11,12; Wei, Peng8; Bird, Sarah A.1,2; Zeng, Shuguang1,2; Huang, Yao1,2; Howell, D. Andrew6,7; Bostroem, K. Azaleee6,7; McCully, Curtis6,7; Hiramatsu, Daichi6,7; Hosseinzadeh, Griffin6,7,13; Li, Wenxiong14; Zhang, Tianmeng15; Wang, Lifan16; Zhou, Guangrong1,2
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| 2023-07-03 | |
| Source Publication | ASTRONOMY & ASTROPHYSICS
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| ISSN | 0004-6361 |
| Volume | 675Pages:A73 |
| Contribution Rank | 7 |
| Abstract | 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. |
| Keyword | supernovae: general supernovae: individual: SN 2018xx supernovae: individual: SN 2019gbx |
| DOI | 10.1051/0004-6361/202244985 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | SPECTRAL ENERGY-DISTRIBUTION ; TIME OPTICAL-SPECTRA ; HOST GALAXIES ; LIGHT CURVES ; SN 2011FE ; IMPROVED DISTANCES ; RISE-TIME ; LUMINOSITY ; METALLICITY ; MODEL |
| Funding Project | 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 Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001022371200010 |
| Publisher | EDP SCIENCES S A |
| Funding Organization | 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) |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5381 |
| Collection | 中国科学院新疆天文台 光学天文与技术应用研究室 |
| Corresponding Author | Zeng, Xiangyun; Wang, Xiaofeng |
| Affiliation | 1.China Three Gorges Univ, Ctr Astron & Space Sci, Yichang 443000, Peoples R China 2.China Three Gorges Univ, Coll Sci, Yichang 443000, Peoples R China 3.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China 4.Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China 5.Beijing Acad Sci Technol, Beijing Planetarium, Beijing 100044, Peoples R China 6.Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA 7.Las Cumbres Observ, 6740 Cortona Dr Suite 102, Goleta, CA 93117 USA 8.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 9.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China 10.Chinese Acad Sci, Yunnan Observ YNAO, Kunming 650216, Peoples R China 11.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650216, Peoples R China 12.Chinese Acad Sci, Ctr Astron Mega Sci, 20A Datun Rd, Beijing, Peoples R China 13.Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA 14.Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel 15.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China 16.Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, Dept Phys & Astron, 4242 TAMU, College Stn, TX 77843 USA |
| Recommended Citation 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:A73. |
| 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,A73. |
| MLA | Li, Yangyang,et al."A comparative analysis of type Ia supernovae 2018xx and 2019gbx".ASTRONOMY & ASTROPHYSICS 675(2023):A73. |
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| Li-2023-A comparativ（3162KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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