Spatially Resolved Spectral Energy Distributions of Nearby Galaxies

Bibcode
2008ASPC..396..157M
Muñoz-Mateos, J. C.; Gil de Paz, A.; Zamorano, J.; Pérez-González, P. G.; Gallego, J.; Boissier, S.; Dale, D. A.; Madore, B. F.; Sánchez, S.
Bibliographical reference

Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at the Centro Convegni Matteo Ricci, Rome, Italy. Edited by José G. Funes, S.J., and Enrico Maria Corsini. San Francisco: Astronomical Society of the Pacific, 2008., p.157

Advertised on:
10
2008
Number of authors
9
IAC number of authors
0
Citations
0
Refereed citations
0
Description
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.
Type
Non-refereed

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