Infrared SED Model for Young Galaxies: Effect of SN Reverse Shock and Shattering on Dust Grains

Details Infrared SED Model for Young Galaxies: Effect of SN Reverse Shock and Shattering on Dust Grains Infrared SED Model for Young Galaxies: Effect of SN Reverse Shock and Shattering on Dust Grains

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1240...91t&link_type=abstract

HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. Edited by Victor P. Debattista and Cristina C. Popescu AIP Conferen

Physics

1

Star Formation, Galaxies, Interstellar Matter, Stellar Mass, Star Formation, Dwarf Galaxies, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Mass And Mass Distribution

Scientific paper

We have developed a model of dust emission from galaxies in their very young phase after the formation. Because of their young age, the primary dust supply is thought to be supernovae (SNe). We present the new IR SED of very young galaxies which includes SN reverse shock destruction and shattering, and show that the obtained SED naturally reproduces the strong mid-IR emission often found in low-metallicity starbursts.

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