The Inflow and Outflow Rate Evolution of Local Milky Way–mass Star-forming Galaxies since z?=?1.3

doi:10.3847/1538-4357/ab11c2

	The Inflow and Outflow Rate Evolution of Local Milky Way–mass Star-forming Galaxies since z?=?1.3
	Pan,Zhizheng 1,2; Peng,Yingjie 3; Zheng,Xianzhong1,2 ; Wang,Jing 3; Kong,Xu 2,4
刊名	The Astrophysical Journal
	2019-04-29
卷号	876 期号:1
关键词	galaxies: evolution
ISSN号	0004-637X
DOI	10.3847/1538-4357/ab11c2
英文摘要	Abstract We study the gas inflow rate (ζinflow) and outflow rate (ζoutflow) evolution of local Milky Way–mass star-forming galaxies (SFGs) since z?=?1.3. The stellar mass growth history of Milky Way–mass progenitor SFGs is inferred from the evolution of the star formation rate (SFR)?stellar mass (M*) relation, and the gas mass (Mgas) is derived using the recently established gas-scaling relations. With the growth curve, the net inflow rate κ is quantified at each cosmic epoch. At z?～?1.3, κ is comparable with the SFR, whereas it rapidly decreases to ～0.15?×?SFR at z?=?0. We then constrain the average outflow rate ζoutflow of progenitor galaxies by modeling the evolution of their gas-phase metallicity. The best-fit ζoutflow is found to be (0.5–0.8)?×?SFR. Combining κ and ζoutflow, we finally investigate the evolution of ζinflow since z?=?1.3. We find that ζinflow rapidly decreases by ～80% from z?=?1.3 to z?=?0.5. At z?
语种	英语
出版者	The American Astronomical Society
WOS记录号	IOP:0004-637X-876-1-AB11C2
内容类型	期刊论文
源URL	[http://libir.pmo.ac.cn/handle/332002/24621]
专题	中国科学院紫金山天文台
作者单位	1.Purple Mountain Observatory, Chinese Academy of Sciences, 8 Yuan Hua Road, Nanjing, Jiangsu 210008, People's Republic of China; panzz@pmo.ac.cn 2.School of Astronomy and Space Sciences, University of Science and Technology of China, Hefei, 230026, People's Republic of China; xzzheng@pmo.ac.cn 3.Kavli Institute for Astronomy and Astrophysics, Peking University, Yi He Yuan Lu 5, Hai Dian District, Beijing 100871, People's Republic of China 4.CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei, Anhui 230026, People's Republic of China; xkong@ustc.edu.cn
推荐引用方式 GB/T 7714	Pan,Zhizheng,Peng,Yingjie,Zheng,Xianzhong,et al. The Inflow and Outflow Rate Evolution of Local Milky Way–mass Star-forming Galaxies since z?=?1.3[J]. The Astrophysical Journal,2019,876(1).
APA	Pan,Zhizheng,Peng,Yingjie,Zheng,Xianzhong,Wang,Jing,&Kong,Xu.(2019).The Inflow and Outflow Rate Evolution of Local Milky Way–mass Star-forming Galaxies since z?=?1.3.The Astrophysical Journal,876(1).
MLA	Pan,Zhizheng,et al."The Inflow and Outflow Rate Evolution of Local Milky Way–mass Star-forming Galaxies since z?=?1.3".The Astrophysical Journal 876.1(2019).