FROM GLOBAL TO SPATIALLY RESOLVED IN LOW-REDSHIFT GALAXIES

被引：45

作者：

Sanchez, S. F. ^{[1
]}

Walcher, C. J. ^{[2
]}

Lopez-Coba, C. ^{[1
]}

Barrera-Ballesteros, J. K. ^{[1
]}

Mejia-Narvaez, A. ^{[1
]}

Espinosa-Ponce, C. ^{[1
]}

Camps-Farina, A. ^{[1
]}

机构：

[1] Univ Nacl Autonoma Mexico, Inst Astron, AP 70-264, Mexico City 04510, DF, Mexico

[2] Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany

来源：

REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA | 2021年 / 57卷 / 01期

基金：

澳大利亚研究理事会; 美国安德鲁·梅隆基金会;

关键词：

Key Words; galaxies; evolution; fundamental parameters; ISM; star formation; stellar content; techniques; imaging spectroscopy; SDSS-IV MANGA; H-II REGIONS; MASS-METALLICITY RELATION; ACTIVE GALACTIC NUCLEUS; STAR-FORMING GALAXIES; DIGITAL SKY SURVEY; STELLAR MASS; PHYSICAL-PROPERTIES; FUNDAMENTAL RELATION; ABUNDANCE GRADIENTS;

D O I：

10.22201/ia.01851101p.2021.57.01.01

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Our understanding of the structure, composition and evolution of galaxies has strongly improved in the last decades, mostly due to new results based on large spectro-scopic and imaging surveys. In particular, the nature of ionized gas, its ionization mech-anisms, its relation with the stellar properties and chemical composition, the existence of scaling relations that describe the cycle between stars and gas, and the corresponding evo-lution patterns have been widely explored and described. More recently, the introduction of additional techniques, in particular integral field spectroscopy, and their use in large galaxy surveys, have forced us to re-interpret most of those recent results from a spatially resolved perspective. This review is aimed to complement recent efforts to compile and summarize this change of paradigm in the interpretation of galaxy evolution. To this end we replicate published results, and present novel ones, based on the largest compilation of IFS data of galaxies in the nearby universe to date.

引用

页码：3 / 38

页数：36

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