Hot dust in galaxies

Details Hot dust in galaxies Hot dust in galaxies

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002pobeo..73...27k&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 73, p. 27 - 36 (2002). In: Proceedings of the Thi

Astronomy and Astrophysics

Astronomy

Galactic Nuclei, Infrared Radiation, Interstellar Dust, Radiative Transfer

Scientific paper

We present an approximate method for calculating the infrared emission from a galactic nucleus that has recently undergone a starburst and is powered mainly by massive stars of spectral type O and B. Such nuclei are usually heavily obscured by dust and we outline the radiative transfer in a dusty medium with scattered sources. We include in the model transiently heated small dust particles and illustrate their dominating influence on the near and mid infrared spectrum.

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