The Evolution of Baryonic Mass Function of Galaxies to z & xfffd;=& xfffd;3
文献类型：期刊论文
| 作者 | Pan, Zhizheng3,4; Peng, Yingjie2; Zheng, Xianzhong3,4; Wang, Jing2; Kong, Xu1,3 |
| 刊名 | ASTROPHYSICAL JOURNAL LETTERS
 |
| 出版日期 | 2019-11-01 |
| 卷号 | 885期号:1页码:5 |
| 关键词 | Galaxy evolution Galaxy quenching |
| ISSN号 | 2041-8205 |
| DOI | 10.3847/2041-8213/ab4bcf |
| 通讯作者 | Pan, Zhizheng(panzz@pmo.ac.cn) |
| 英文摘要 | We combine the published stellar mass function (SMF) and gas scaling relations to explore the baryonic (stellar plus cold gas) mass function (BMF) of galaxies to redshift z = 3. We find evidence that at log(M-baryon/M-circle dot).> 11.3, the BMF has evolved little since z similar to 2.2. With the evolution of BMF and SMF, we investigate the baryon net accretion rate ((rho) over dot(baryon)) and stellar mass growth rate ((rho) over dot(star)) for the galaxy population of log(M-star/M-circle dot) > 10. The ratio between these two quantities, (rho)over dot(baryon)/(rho)over dot(star), decreases from (rho)over dot(baryon)/(rho)over dot(star) similar to 2 at z similar to 2.5 to (rho) over dot(baryon)/(rho) over dot(star) < 0.5 at z similar to 0.5, suggesting that massive galaxies are transforming from the "accretion-dominated" phase to the "depletion-dominated" phase from high-z to low-z. The transition of these two phases occurs at z similar to 1.5, which is consistent with the onset redshift of the decline of cosmic star formation rate density (CSFD). This provides evidence to support the idea that the decline of CSFD since z similar to 1.5 mainly results from the decline of baryon net accretion rate and star formation quenching in galaxies. |
| WOS关键词 | STAR-FORMING GALAXIES ; METALLICITY RELATION ; MAIN-SEQUENCE ; GAS ; FLOWS ; STELLAR ; ORIGIN ; COSMOS ; MODEL |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000498628300005 |
| 出版者 | IOP PUBLISHING LTD |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/35138]  |
| 专题 | 中国科学院紫金山天文台 |
| 通讯作者 | Pan, Zhizheng |
| 作者单位 | 1.Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China 2.Peking Univ, Kavli Inst Astron & Astrophys, Yi He Yuan Lu 5, Beijing 100871, Peoples R China 3.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R China 4.Chinese Acad Sci, Purple Mt Observ, 10 Yuan Hua Rd, Nanjing 210033, Jiangsu, Peoples R China |
| 推荐引用方式 GB/T 7714 | Pan, Zhizheng,Peng, Yingjie,Zheng, Xianzhong,et al. The Evolution of Baryonic Mass Function of Galaxies to z & xfffd;=& xfffd;3[J]. ASTROPHYSICAL JOURNAL LETTERS,2019,885(1):5. |
| APA | Pan, Zhizheng,Peng, Yingjie,Zheng, Xianzhong,Wang, Jing,&Kong, Xu.(2019).The Evolution of Baryonic Mass Function of Galaxies to z & xfffd;=& xfffd;3.ASTROPHYSICAL JOURNAL LETTERS,885(1),5. |
| MLA | Pan, Zhizheng,et al."The Evolution of Baryonic Mass Function of Galaxies to z & xfffd;=& xfffd;3".ASTROPHYSICAL JOURNAL LETTERS 885.1(2019):5. |
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来源：紫金山天文台
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