ASCA observations of ultra luminous infrared galaxies - evolution from starburst to AGN?

被引：0
|
作者：
Nakagawa, T
Kii, T
Fujimoto, R
Miyazaki, T
Inoue, H
Ogasaka, Y
Ikebe, Y
Kawabe, R
机构：
[1] Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
[2] Nagoya Univ, Nagoya, Aichi 4648602, Japan
[3] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
[4] Nobeyama Radio Observ, Nagano 3841305, Japan
来源：
ASTRONOMISCHE NACHRICHTEN | 1999年 / 320卷 / 4-5期
关键词：
ultra luminous infrared galaxies;
D O I：
10.1002/1521-3994(199908)320:4/5<246::AID-ASNA246>3.0.CO;2-S
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We made a series of ASCA observations of Ultra Luminous Infrared Galaxies (ULIRGs), to reveal the origin of their luminosities and to test a proposed evolutionary scenario of ULIRGs. We discovered embedded AGN in some galaxies, but the relative contribution of AGN activity to the total luminosity varies significantly from galaxy to galaxy and has no correlation with the evolutionary sequence as mergers.
引用
收藏
页码：246 / 247
页数：2
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