The ALMaQUEST survey - III. Scatter in the resolved star-forming main sequence is primarily due to variations in star formation efficiency

被引:60
|
作者
Ellison, Sara L. [1 ]
Thorp, Mallory D. [1 ]
Lin, Lihwai [2 ]
Pan, Hsi-An [2 ]
Bluck, Asa F. L. [3 ]
Scudder, Jillian M. [4 ]
Teimoorinia, Hossen [1 ,5 ]
Sanchez, Sebastian F. [6 ]
Sargent, Mark [7 ]
机构
[1] Univ Victoria, Dept Phys & Astron, Finnerty Rd, Victoria, BC V8P 1A1, Canada
[2] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan
[3] Univ Cambridge, Kavli Inst Cosmol & Cavendish Astrophys, Madingley Rd, Cambridge CB3 0HA, England
[4] Oberlin Coll, Dept Phys & Astron, Oberlin, OH 44074 USA
[5] NRC Herzberg Astron & Astrophys, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada
[6] Univ Nacl Autonoma Mexico, Inst Astron, AP 70-264, Mexico City 04510, DF, Mexico
[7] Univ Sussex, Astron Ctr, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England
基金
欧洲研究理事会;
关键词
galaxies: evolution; galaxies: general; galaxies: ISM; galaxies: star formation; FORMATION RATES; NEARBY GALAXIES; MOLECULAR GAS; FORMATION LAW; MASS; II;
D O I
10.1093/mnrasl/slz179
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using a sample of 11 478 spaxels in 34 galaxies with molecular gas, star formation, and stellar maps taken from the ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) survey, we investigate the parameters that correlate with variations in star formation rates on kpc scales. We use a combination of correlation statistics and an artificial neural network to quantify the parameters that drive both the absolute star formation rate surface density (Sigma(SFR)), as well as its scatter around the resolved star-forming main sequence (Delta Sigma(SFR)). We find that Est is primarily regulated by molecular gas surface density (EH2) with a secondary dependence on stellar mass surface density (Sigma(*)), as expected from an 'extended Kennicutt-Schmidt relation'. However, Delta Sigma(SFR) is driven primarily by changes in star formation efficiency (SFE), with variations in gas fraction playing a secondary role. Taken together, our results demonstrate that whilst the absolute rate of star formation is primarily set by the amount of molecular gas, the variation of star formation rate above and below the resolved star-forming main sequence (on kpc scales) is primarily due to changes in SFE.
引用
收藏
页码:L39 / L43
页数:5
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