Morphology of Nearby Galaxies

被引：0

作者：

Buta, Ronald J. ^{[1
]}

机构：

[1] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA

来源：

STRUCTURE AND DYNAMICS OF DISK GALAXIES | 2014年 / 480卷

关键词：

DIGITAL-SKY-SURVEY; STAR-FORMATION RATES; POLAR-RING GALAXIES; SECULAR EVOLUTION; STELLAR STRUCTURE; HUBBLE SEQUENCE; SPIRAL GALAXIES; SPITZER SURVEY; CLASSIFICATION-SYSTEM; ELLIPTIC GALAXIES;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Improved knowledge of the morphology of nearby galaxies has resulted from large imaging surveys such as the Sloan Digital Sky Survey (SDSS; optical wavelengths), the Galaxy Evolution Explorer (GALEX; near- and far-ultraviolet wavelengths), and the Spitzer Survey of Stellar Structure in Galaxies (S4G; mid-infrared wavelengths). In this review, I summarize the basic aspects of nearby galaxy morphology and highlight the strength of the morphological survey as a means of learning more about how galaxies are structured and how they might evolve.

引用

页码：53 / 64

页数：12

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