Metallicity calibrations and oxygen abundance evolution in massive galaxies

被引：0

作者：

Maliuk, A. A. ^{[1
]}

Zinchenko, I. A. ^{[2
]}

机构：

[1] Taras Shevchenko Natl Univ Kyiv, Glushkova Ave 4, UA-03127 Kiev, Ukraine

[2] NAS Ukraine, Main Astron Observ, 27 Akad Zabolotnoho Str, UA-03143 Kiev, Ukraine

来源：

ADVANCES IN ASTRONOMY AND SPACE PHYSICS | 2018年 / 8卷 / 01期

基金：

美国安德鲁·梅隆基金会; 美国国家科学基金会;

关键词：

ISM: HII regions - galaxies: abundances; evolution;

D O I：

10.17721/2227-1481.8.24-27

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We determined oxygen abundances for the sample of SDSS galaxies with high masses using R-3D, S-3D, R-2D, S-2D, N and O3N2 calibrations. We investigated redshift-metallicity relation for oxygen abundances obtained by each calibration. We found that for galaxies with high stellar masses oxygen abundance obtained using all calibrations is increasing on the time interval from z = 0.5 to z = 0. However, the values of oxygen abundance enrichment rate significantly depend on adopted calibration and ranges from similar to 0.1 dex per unit redshift for R calibration to similar to 0.5 dex per unit redshift for O3N2 calibration.

引用

页码：24 / 27

页数：4

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