Spatially Resolved Spectral Energy Distributions of Nearby Galaxies

被引：0
|
作者：
Munoz-Mateos, J. C. [1 ]
Gil de Paz, A. [1 ]
Zamorano, J. [1 ]
Perez-Gonzalez, P. G. [1 ]
Gallego, J. [1 ]
Boissier, S. [2 ]
Dale, D. A. [3 ]
Madore, B. F. [4 ]
Sanchez, S.
机构：
[1] Univ Complutense Madrid, Dept Astrofis, Madrid, Spain
[2] Lab Astrophys Marseille, Marseille, France
[3] Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA
[4] Carnegie Inst Sci, Pasadena, CA USA
来源：
FORMATION AND EVOLUTION OF GALAXY DISKS | 2008年 / 396卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present azimuthally-averaged spectral energy distributions (SEDs) from FUV to FIR, as a function of radius, for the galaxies included in the SINGS sample. The radial changes in these SEDs are interpreted in terms of variations of the relative contribution of stars (of different ages), dust and gas.
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页码：157 / +
页数：2
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