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Paper: Dust SED Model of Very Young Galaxies with AGB-Star Dust
Volume: 445, Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants
Page: 551
Authors: Takeuchi, T. T.; Asano, R. S.; Ishii, T. T.; Nozawa, T.; Hirashita, H.; Kozasa, T.
Abstract: Recently, it has been found that the contribution of dust from AGB stars is significant even if the galaxy is very young (age < 1 Gyr). We show a dust SED model including the emission from dust from AGB stars based on our new dust evolution scenario. The AGB-star dust contribution increases the infrared luminosity of galaxies after the age of several × 108 yr.
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