|
|
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. |
|
|
|
|