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.
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页码：53 / 64
页数：12
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