| Discovery and Extensive Follow-up of SN 2024ggi, a Nearby Type IIP Supernova in NGC 3621 | |
Chen, Ting-Wan1; Yang, Sheng2; Srivastav, Shubham3; Moriya, Takashi J.4,5,6; Smartt, Stephen J.3,7; Rest, Sofia8; Rest, Armin9,10; Lin, Hsing Wen11; Miao, Hao-Yu1; Cheng, Yu-Chi12,13; Aryan, Amar1; Cheng, Chia-Yu1; Fraser, Morgan14; Huang, Li-Ching12,13; Lee, Meng-Han1; Lai, Cheng-Han1; Liu, Yu-Hsuan1,15; Sankar.K, Aiswarya1; Smith, Ken W.7; Stevance, Heloise F.3,7; Wang, Ze-Ning2,16; Anderson, Joseph P.17,18; Angus, Charlotte R.7; Boer, Thomas de19; Chambers, Kenneth19; Duan, Hao-Yuan20; Erasmus, Nicolas21; Fulton, Michael7; Gao, Hua19; Herman, Joanna19; Hou, Wei-Jie1; Hsiao, Hsiang-Yao1; Huber, Mark E.19; Lin, Chien-Cheng19; Lin, Hung-Chin1; Magnier, Eugene A.19; Man, Ka Kit22; Moore, Thomas7,17; Ngeow, Chow-Choong1; Nicholl, Matt7; Ou, Po-Sheng15,23; Pignata, Giuliano18,24; Shiau, Yu-Chien25; Sommer, Julian Silvester26; Tonry, John L.19; Wang, Xiao-Feng27,28; Wainscoat, Richard19; Young, David R.7; Yeh, You-Ting29; Zhang JJ(张居甲)30,31
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| 发表期刊 | ASTROPHYSICAL JOURNAL
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| 2025-04-10 | |
| 卷号 | 983期号:1 |
| DOI | 10.3847/1538-4357/adb428 |
| 产权排序 | 第30完成单位 |
| 收录类别 | SCI |
| 摘要 | We present the discovery and early observations of the nearby Type II supernova (SN) 2024ggi in NGC 3621 at 6.64 +/- 0.3 Mpc. The SN was caught 5.8-2.9+1.9 hr after its explosion by the ATLAS survey. Early-phase, high-cadence, and multiband photometric follow-up was performed by the Kilonova Finder (Kinder) project, collecting over 1000 photometric data points within 1 week. The combined o- and r-band light curves show a rapid rise of 3.3 mag in 13.7 hr, much faster than SN 2023ixf (another nearby and well-observed SN II). Between 13.8 and 18.8 hr after explosion, SN 2024ggi became bluer, with u - g color dropping from 0.53 to 0.15 mag. The rapid blueward evolution indicates a wind shock breakout (SBO) scenario. No hour-long brightening expected for the SBO from a bare stellar surface was detected during our observations. The classification spectrum, taken 17 hr after the SN explosion, shows flash features of high-ionization species such as Balmer lines, He i, C iii, and N iii. Detailed light-curve modeling provides critical insights into the circumstellar material (CSM). Our favored model has an explosion energy of 2 x 1051 erg, a mass-loss rate of 10-3 M circle dot yr-1 (with an assumed 10 km s-1 wind), and a confined CSM radius of 6 x 1014 cm. The corresponding CSM mass is 0.4 M circle dot. Comparisons with SN 2023ixf highlight that SN 2024ggi has a less dense confined CSM, resulting in a faster rise and fainter UV flux. Citizen astronomer collaboration and extensive data are essential for SBO searches and detailed SN characterizations. |
| 资助项目 | Ministry of Education, Taiwan[MOE-111-YSFMS-0008-001-P1]; National Natural Science Foundation of China[12173082]; Henan Province High-Level Talent International Training Program; JSPS Core-to-Core Program[JPJSCCA20210003]; Millennium Science Initiative[ICN12_009]; Royal Society-Science Foundation Ireland University Research Fellowship; European Research Council (ERC) under the European Union[948381]; UK Space Agency[ST/Y000692/1]; UK Space Agency[ICN12 009]; Eric and Wendy Schmidt AI in Science Fellowship; Tencent Xplorer Prize; National Key R&D Program of China[2021YFA1600404]; Yunnan Province Foundation[202201AT070069]; Top-notch Young Talents Program of Yunnan Province; Chinese Academy of Sciences; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001]; Asteroid Terrestrial-impact Last Alert System (ATLAS) project; Asteroid Terrestrial-impact Last Alert System (ATLAS) project is primarily funded to search for near-Earth asteroids through NASA[NN12AR55G]; Asteroid Terrestrial-impact Last Alert System (ATLAS) project is primarily funded to search for near-Earth asteroids through NASA[80NSSC18K0284]; Asteroid Terrestrial-impact Last Alert System (ATLAS) project is primarily funded to search for near-Earth asteroids through NASA[80NSSC18K1575]; Asteroid Terrestrial-impact Last Alert System (ATLAS) project is primarily funded to search for near-Earth asteroids through NASA[J1944/80NSSC19K0112]; Asteroid Terrestrial-impact Last Alert System (ATLAS) project is primarily funded to search for near-Earth asteroids through NASA[HST GO-15889]; STFC[ST/T000198/1]; STFC[ST/S006109/1]; Queen's University Belfast; South African Astronomical Observatory; Pan-STARRS Project Office; Max Planck Society; Max Planck Institute for Extraterrestrial Physics; National Central University of Taiwan; Space Telescope Science Institute; National Aeronautics and Space Administration[NNX08AR22G]; NASA Science Mission Directorate; National Science Foundation[AST-1238877]; University of Maryland, Eotvos Lorand University (ELTE); Los Alamos National Laboratory; Gordon and Betty Moore Foundation; NASA[NAS 5-26555]; MoST grant[109-2112-M-008-001] |
| 项目资助者 | Ministry of Education, Taiwan[MOE-111-YSFMS-0008-001-P1] ; National Natural Science Foundation of China[12173082] ; Henan Province High-Level Talent International Training Program ; JSPS Core-to-Core Program[JPJSCCA20210003] ; Millennium Science Initiative[ICN12_009] ; Royal Society-Science Foundation Ireland University Research Fellowship ; European Research Council (ERC) under the European Union[948381] ; UK Space Agency[ST/Y000692/1, ICN12 009] ; Eric and Wendy Schmidt AI in Science Fellowship ; Tencent Xplorer Prize ; National Key R&D Program of China[2021YFA1600404] ; Yunnan Province Foundation[202201AT070069] ; Top-notch Young Talents Program of Yunnan Province ; Chinese Academy of Sciences ; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001] ; Asteroid Terrestrial-impact Last Alert System (ATLAS) project ; Asteroid Terrestrial-impact Last Alert System (ATLAS) project is primarily funded to search for near-Earth asteroids through NASA[NN12AR55G, 80NSSC18K0284, 80NSSC18K1575, J1944/80NSSC19K0112, HST GO-15889] ; STFC[ST/T000198/1, ST/S006109/1] ; Queen's University Belfast ; South African Astronomical Observatory ; Pan-STARRS Project Office ; Max Planck Society ; Max Planck Institute for Extraterrestrial Physics ; National Central University of Taiwan ; Space Telescope Science Institute ; National Aeronautics and Space Administration[NNX08AR22G] ; NASA Science Mission Directorate ; National Science Foundation[AST-1238877] ; University of Maryland, Eotvos Lorand University (ELTE) ; Los Alamos National Laboratory ; Gordon and Betty Moore Foundation ; NASA[NAS 5-26555] ; MoST grant[109-2112-M-008-001] |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 恒星与银河系 |
| 文章类型 | Article |
| 出版者 | IOP Publishing Ltd |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| ISSN | 0004-637X |
| URL | 查看原文 |
| WOS记录号 | WOS:001462690500001 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | NUCLEAR STAR-CLUSTERS ; CIRCUMSTELLAR-MATERIAL ; SHOCK BREAKOUT ; LIGHT CURVES ; MASSES ; PROGENITOR ; EXPLOSION ; CLASSIFICATION ; TELESCOPE ; EMISSION |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 版本 | 出版稿 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/28255 |
| 专题 | 南方基地 |
| 作者单位 | 1.Graduate Institute of Astronomy, National Central University, 300 Jhongda Road, 32001 Jhongli, Taiwan; [email protected]; 2.Henan Academy of Sciences, Zhengzhou 450046, Henan, People's Republic of China; [email protected]; 3.Astrophysics Sub-Department, Department of Physics, University of Oxford, Keble Road, Oxford, OX1 3RH, UK; 4.National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; 5.Graduate Institute for Advanced Studies, SOKENDAI, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; 6.School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia; 7.Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, BT7 1NN, UK; 8.Department of Computer Science, The Johns Hopkins University, Baltimore, MD 21218, USA; 9.Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA; 10.Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, USA; 11.Department of Physics, University of Michigan, 450 Church Street, Ann Arbor, MI 48109-1107, USA; 12.Department of Physics, National Taiwan Normal University, No. 88, Sect. 4, Tingzhou Road, Wenshan Dist., Taipei City, 116325, Taiwan; 13.Center of Astronomy and Gravitation, National Taiwan Normal University, No. 88, Sect. 4, Tingzhou Road, Wenshan Dist., Taipei City, 116325, Taiwan; 14.School of Physics, O'Brien Centre for Science North, University College Dublin, Belfield, Dublin 4, Ireland; 15.Institute of Astronomy and Astrophysics, Academia Sinica, No. 1, Sec. 4, Roosevelt Road, Taipei 106216, Taiwan; 16.School of Physics, Henan Normal University, Xinxiang 453007, Henan, People's Republic of China; 17.European Southern Observatory, Alonso de Córdova 3107, Casilla 19, Santiago, Chile; 18.Millennium Institute of Astrophysics MAS, Nuncio Monseñor Sotero Sanz 100, Off. 104, Providencia, Santiago, Chile; 19.Institute for Astronomy, University of Hawai'i, 2680 Woodlawn Drive, Honolulu, HI 96822, USA; 20.Taipei Astronomical Museum, Taipei, Taiwan; 21.South African Astronomical Observatory, 1 Observatory Road, Cape Town, 7925, South Africa; 22.School of Business, Hong Kong Baptist University, Hong Kong; 23.Department of Physics, National Taiwan University, No. 1, Sec. 4, Roosevelt Road, Taipei 106216, Taiwan; 24.Instituto de Alta Investigación, Universidad de Tarapacá, Casilla 7D, Arica, Chile; 25.Taipei Amateur Astronomers Association; 26.Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität, Scheinerstr. 1, 81679 München, Germany; 27.Physics Department, Tsinghua University, Beijing, 100084, People's Republic of China; 28.Purple Mountain Observatory, Chinese Academy of Science, Nanjing, 210023, People's Republic of China; 29.CheCheng Elementary School Observatory, Taiwan; 30.Yunnan Observatories (YNAO), Chinese Academy of Sciences (CAS), Kunming, 650216, People's Republic of China; 31.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China |
| 推荐引用方式 GB/T 7714 | Chen, Ting-Wan,Yang, Sheng,Srivastav, Shubham,et al. Discovery and Extensive Follow-up of SN 2024ggi, a Nearby Type IIP Supernova in NGC 3621[J]. ASTROPHYSICAL JOURNAL,2025,983(1). |
| APA | Chen, Ting-Wan.,Yang, Sheng.,Srivastav, Shubham.,Moriya, Takashi J..,Smartt, Stephen J..,...&张居甲.(2025).Discovery and Extensive Follow-up of SN 2024ggi, a Nearby Type IIP Supernova in NGC 3621.ASTROPHYSICAL JOURNAL,983(1). |
| MLA | Chen, Ting-Wan,et al."Discovery and Extensive Follow-up of SN 2024ggi, a Nearby Type IIP Supernova in NGC 3621".ASTROPHYSICAL JOURNAL 983.1(2025). |
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