Infrared SEDs and the Local Environment within Star-Forming Galaxies

Details Infrared SEDs and the Local Environment within Star-Forming Galaxies Infrared SEDs and the Local Environment within Star-Forming Galaxies

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..761..380d&link_type=abstract

THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP Conference Pr

Astronomy and Astrophysics

Astronomy

1

Origin, Formation, Evolution, Age, And Star Formation, Infrared Emission, Infrared

Scientific paper

The Spitzer Infrared Nearby Galaxies Survey (SINGS) is carrying out a comprehensive multi-wavelength survey on a sample of 75 nearby galaxies. Infrared data from the Spitzer Space Telescope are now becoming available for several sources in the SINGS sample. We present a preliminary analysis on the shape and variations of the infrared spectral energy distributions as a function of position, within the context of the previous generation of models that were developed based on global Infrared Space Observatory and Infrared Astronomical Satellite data for normal star-forming galaxies. Correlations with the properties of the underlying local environment are explored.

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