CO-EVOLUTION OF SUPERMASSIVE BLACK HOLES AND GALAXIES IN THE NEAR UNIVERSE

被引：0
|
作者：
Riffel, R. A. [1 ]
Storchi-Bergmann, T. [2 ]
机构：
[1] Univ Fed Santa Maria, Dept Fis, CCNE, BR-97105900 Santa Maria, RS, Brazil
[2] Univ Fed Rio Grande do Sul, IF, BR-91501970 Porto Alegre, RS, Brazil
来源：
XIV LATIN AMERICAN REGIONAL IAU MEETING | 2014年 / 44卷
关键词：
GEMINI NIFS; FEEDBACK; NUCLEUS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Although the bulk of the. supermassive black hole (SMBH) growth has occurred at red shifts higher than 2, the feeding processes cannot be resolved at the corresponding distances. It is in the near Universe that these processes - which take place within the inner few hundred parsecs of active galaxies can be probed down to similar to 10 pc spatial resolution. We discuss integral field spectroscopic observations of the inner kiloparsec of nearby active galaxies which reveal the presence of gas reservoirs and inflows along nuclear spirals and filaments.
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收藏
页码：102 / 102
页数：1
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