From Haloes to Galaxies. II. The Fundamental Relations in Star Formation and Quenching
文献类型:期刊论文
作者 | Dou,Jing15,16; Peng,Yingjie15; Renzini,Alvio1; Ho,Luis C.15,16; Mannucci,Filippo2; Daddi,Emanuele11; Gao,Yu5,6; Maiolino,Roberto4,12,14; Zhang,Chengpeng15,16; Gu,Qiusheng8,9 |
刊名 | The Astrophysical Journal |
出版日期 | 2021-02-01 |
卷号 | 907期号:2 |
ISSN号 | 0004-637X |
关键词 | Galaxy evolution Star formation Interstellar medium Galaxy formation |
DOI | 10.3847/1538-4357/abd17c |
英文摘要 | Abstract Star formation and quenching are two of the most important processes in galaxy formation and evolution. We explore in the local universe the interrelationships among key integrated galaxy properties, including stellar mass M*, star formation rate (SFR), specific SFR (sSFR), molecular gas mass M H 2 , star formation efficiency (SFE) of the molecular gas, and the molecular gas to stellar mass ratio μ. We aim to identify the most fundamental scaling relations among these key galaxy properties and their interrelationships. We show that the integrated M H 2 –SFR, SFR–M*, and M H 2 –M* relations can be simply transformed from the μ–sSFR, SFE–μ, and SFE–sSFR relations, respectively. The transformation, in principle, can increase or decrease the scatter of each relation. Interestingly, we find that the latter three relations all have significantly smaller scatter than the corresponding former three. We show that the probability to achieve the observed small scatter by accident is extremely close to zero. This suggests that the smaller scatters of the latter three relations are driven by a more universal physical connection among these quantities. We then show that the large scatters in the former relations are due to their systematic dependence on other galaxy properties, and on the star formation and quenching process. We propose the sSFR–μ–SFE relation as the fundamental formation relation (FFR), which governs the star formation and quenching process and provides a simple framework to study galaxy evolution. Other scaling relations, including the integrated Kennicutt–Schmidt law, star-forming main sequence, and molecular gas main sequence, can all be derived from the FFR. |
语种 | 英语 |
出版者 | The American Astronomical Society |
WOS记录号 | IOP:0004-637X-907-2-ABD17C |
源URL | [http://ir.bao.ac.cn/handle/114a11/60427] |
专题 | 中国科学院国家天文台 |
通讯作者 | Dou,Jing; Peng,Yingjie |
作者单位 | 1.INAF—Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, I-35122 Padova, Italy 2.Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy 3.Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland 4.Cavendish Laboratory, University of Cambridge, 19 J.J. Thomson Avenue, Cambridge CB3 0HE, UK 5.Department of Astronomy, Xiamen University, Xiamen, Fujian 361005, People’s Republic of China 6.Purple Mountain Observatory & Key Laboratory for Radio Astronomy, Chinese Academy of Sciences, 10 Yuanhua Road, Nanjing 210033, People’s Republic of China 7.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, People’s Republic of China 8.School of Astronomy and Space Science, Nanjing University, Nanjing 210093, People’s Republic of China 9.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, People’s Republic of China 10.CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China |
推荐引用方式 GB/T 7714 | Dou,Jing,Peng,Yingjie,Renzini,Alvio,et al. From Haloes to Galaxies. II. The Fundamental Relations in Star Formation and Quenching[J]. The Astrophysical Journal,2021,907(2). |
APA | Dou,Jing.,Peng,Yingjie.,Renzini,Alvio.,Ho,Luis C..,Mannucci,Filippo.,...&Yuan,Feng.(2021).From Haloes to Galaxies. II. The Fundamental Relations in Star Formation and Quenching.The Astrophysical Journal,907(2). |
MLA | Dou,Jing,et al."From Haloes to Galaxies. II. The Fundamental Relations in Star Formation and Quenching".The Astrophysical Journal 907.2(2021). |
入库方式: OAI收割
来源:国家天文台
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