期刊
ASTRONOMISCHE NACHRICHTEN
卷 330, 期 9-10, 页码 888-897出版社
WILEY-V C H VERLAG GMBH
DOI: 10.1002/asna.200911256
关键词
galaxies: clusters: general; galaxies: evolution; galaxies: ISM; galaxies: spiral; intergalactic medium
While galaxies move through the intracluster medium of their host cluster, they experience a ram pressure which removes at least a significant part of their interstellar medium. This ram pressure stripping appears to be especially important for spiral galaxies: this scenario is a good candidate to explain the differences observed between cluster spirals in the nearby universe and their field counterparts. Thus, ram pressure stripping of disk galaxies in clusters has been studied intensively during the last decade. I review advances made in this area, concentrating on theoretical work, but continuously comparing to observations. (C) 2009 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据