Model for Infrared Properties of Extremely Young Galaxies

Details Model for Infrared Properties of Extremely Young Galaxies Model for Infrared Properties of Extremely Young Galaxies

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..217..214t&link_type=abstract

International Astronomical Union Symposium no. 217, held 14-17 July, 2003 in Sydney, Australia. Edited by P.-A. Duc, J. Braine

Astronomy and Astrophysics

Astronomy

Scientific paper

We constructed a model of the infrared spectral energy distribution for
very young galaxies by taking into account the dust size distribution in
the early stage of galaxy evolution.

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