No CrossRef data available.
Article contents
Cold HI Gas in the M17SW Giant Molecular Cloud
Published online by Cambridge University Press: 25 April 2016
Abstract
The cold HI cloud in the region of the M17SW giant molecular cloud comprises three major fragments with a mean size of ~ 30 pc. Their overall distribution is rather similar to that of CO gas, but one of the fragments does not seem to have a molecular counterpart. It is shown that such a cloud is also a future site of star formation.
- Type
- Galactic and Stellar
- Information
- Copyright
- Copyright © Astronomical Society of Australia 1991