Mass-metallicity relation for AKARI-FMOS infrared luminous galaxies at z ∼ 0.9

被引：0
|
作者：
Oi, Nagisa [1 ]
Matsuhara, Hideo [1 ]
Goto, Tomotsugu [2 ]
Pearson, Chris [3 ]
Buat, Veronique [4 ]
Malkan, Matthew A. [5 ]
机构：
[1] JAXA ISAS, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan
[2] Natl Tsing Hua Univ, Hsinchu, Taiwan
[3] Univ Oxford, Oxford Astrophys, Oxford, England
[4] Lab Astrophys Marseille, Marseille, France
[5] Univ Calif Los Angeles, Los Angeles, CA USA
来源：
FROM INTERSTELLAR CLOUDS TO STAR-FORMING GALAXIES: UNIVERSAL PROCESSES? | 2015年 / 315期
关键词：
galaxies: evolution; galaxies: fundamental parameter (metallicity); infrared: galaxies; STAR-FORMATION; CATALOG;
D O I：
10.1017/S1743921316008206
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We study the mass-metallicity relation and fundamental relation (FMR) for infrared bright galaxies (IR galaxies) at z similar to 0.9 discovered by AKARI NEP-Deep survey. The main result of this work is that metallicity of IR galaxies surprisingly match optical selected galaxies at a given mass even their star formation rates are different, which may imply that optical and IR selected galaxies follow similar star formation histories, and the starbursts in the IR galaxies do not give a strong impact in changing metallicity because of the short duration time.
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