Research Project
Grant-in-Aid for Scientific Research (C)
Ammonia spectral line observations were conducted to survey dense molecular gas in the Galactic star forming regions. Molecular gas temperature derived from the observations was related to star formation activity, which suggested that active star formation heated the gas. Moreover, molecular gas was hot in a cloud scale in one of the extremely active star forming regions. It was also appeared that molecular gas properties and thus star formation were affected through gas kinematics in a galactic scale.
All 2010 2009 2008 2007
All Journal Article (6 results) (of which Peer Reviewed: 6 results) Presentation (39 results)
北海道大学学位論文
北海道大学 学位論文
Publications of the Astronomical Society of Japan Vol. 60, No. 6
Pages: 1285-1296
10023915670
Publications of the Astronomical Society of Japan 60