Infrared/Submillimeter Continuum Emission of Dust in Galaxies

Details Infrared/Submillimeter Continuum Emission of Dust in Galaxies Infrared/Submillimeter Continuum Emission of Dust in Galaxies

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..309..179d&link_type=abstract

Astrophysics of Dust, ASP Conference Series, Vol. 309,Proceedings of the conference held 26-30 May, 2003 in Estes Park, Colorado

Astronomy and Astrophysics

Astrophysics

Scientific paper

A wealth of new data from infrared and submillimeter telescopes has spurred progress in the study of galaxy spectral energy distributions at long wavelengths. In this contribution I focus on recent semi-empirical work in modeling galaxy infrared spectral energy distributions. A range of applications and topics are discussed including the environmental impact on dust emissivity, the utility of infrared-based photometric redshifts, and the possibilities that will arise with the advent of SIRTF.

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