CHARACTERIZING DUST ATTENUATION IN LOCAL STAR-FORMING GALAXIES: UV AND OPTICAL REDDENING

被引：62
|
作者：
Battisti, A. J. [1 ]
Calzetti, D. [1 ]
Chary, R. -R. [2 ]
机构：
[1] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
[2] CALTECH, US Planck Data Ctr, MS314-6,1200 East Calif Blvd, Pasadena, CA 91125 USA
来源：
ASTROPHYSICAL JOURNAL | 2016年 / 818卷 / 01期
基金：
美国国家航空航天局; 美国国家科学基金会;
关键词：
dust; extinction; galaxies: evolution; galaxies: general; galaxies: ISM; DIGITAL SKY SURVEY; SIMILAR-TO; 2; MASS-METALLICITY RELATION; HIGH-REDSHIFT GALAXIES; ACTIVE GALACTIC NUCLEI; SMALL-MAGELLANIC-CLOUD; ULTRAVIOLET EXTINCTION; STARBURST GALAXIES; INTERSTELLAR DUST; FORMATION HISTORY;
D O I：
10.3847/0004-637X/818/1/13
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The dust attenuation for a sample of 10,000 local (z less than or similar to 0.1) star-forming galaxies is constrained as a function of their physical properties. We utilize aperture-matched multiwavelength data available from the Galaxy Evolution Explorer and the Sloan Digital Sky Survey to ensure that regions of comparable size in each galaxy are being analyzed.
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页数：24
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