Spatially Resolved Spectral Energy Distributions of Nearby Galaxies

Details Spatially Resolved Spectral Energy Distributions of Nearby Galaxies Spatially Resolved Spectral Energy Distributions of Nearby Galaxies

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..396..157m&link_type=abstract

Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at

Astronomy and Astrophysics

Astronomy

Scientific paper

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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