Spectroscopy of galactic winds in ultraluminous infrared galaxies at 0.1 z < 0.5

被引：0
|
作者：
Rupke, DS [1 ]
Veilleux, S [1 ]
Sanders, DB [1 ]
机构：
[1] Univ Maryland, College Pk, MD 20740 USA
来源：
NEUTRAL ISM IN STARBURST GALAXIES | 2004年 / 320卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Galactic winds are a ubiquitous phenomenon in local and high-redshift star-forming galaxies, but they have not been studied in much detail outside of the very local universe. We present preliminary results of a study of massive outflows in a large sample of starburst-dominated ultraluminous infrared galaxies at low to intermediate redshifts (z = 0.1 - 0.5). The technique is absorption-line spectroscopy, and we find winds in the majority of our sample. We also find a correlation of 'mass entrainment efficiency' with star formation rate. Ours is the first systematic, large-scale study of galactic winds in this redshift range.
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页码：307 / 310
页数：4
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