Dust SED Model of Very Young Galaxies with AGB-Star Dust

被引：0

作者：

Takeuchi, T. T. ^{[1
]}

Asano, R. S. ^{[2
]}

Ishii, T. T. ^{[3
]}

Nozawa, T. ^{[4
]}

Hirashita, H. ^{[5
]}

Kozasa, T. ^{[6
]}

机构：

[1] Nagoya Univ, Inst Adv Res, Nagoya, Aichi 4648601, Japan

[2] Nagoya Univ, Dept Phys, Nagoya, Aichi 4648601, Japan

[3] Kyoto Univ, Kwasan Observ, Kyoto 6068501, Japan

[4] Univ Tokyo, IPMU, Tokyo 1138654, Japan

[5] Acad Sinica, Inst Astron & Astrophys, Taipei, Taiwan

[6] Hokkaido Univ, Dept Cosmosci, Sapporo, Hokkaido 060, Japan

来源：

WHY GALAXIES CARE ABOUT AGB STARS II: SHINING EXAMPLES AND COMMON INHABITANTS | 2011年 / 445卷

关键词：

UNIVERSE; GRAINS; EJECTA;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 x 10(8) yr.

引用

页码：551 / +

页数：2

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