首页 | 本学科首页   官方微博 | 高级检索  
     检索      


The Origin of the H I Holes in the Interstellar Medium of Holmberg II
Authors:Sami Dib  Andreas Burkert
Institution:1. Max-Planck-Institut für Astronomie, Heidelberg, Germany
Abstract:We use a comparison between the autocorrelation length value in 21-cm hi maps of Holmberg II and the autocorrelation length derived from simulated maps in order to constrain the physical processes that are responsible for the observed distribution of holes and shells in the interstellar medium (ISM) of the galaxy. Our results show that large scale turbulence coupled to a weak cooling can reproduce the value of the autocorrelation length which is observed.
Keywords:
本文献已被 SpringerLink 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号