Chapter
Studies of Star Forming Regions in M33
Abstract
Molecular clouds similar to Galactic Giant Molecular Clouds have been detected in six of seven fields mapped with the Owens Valley interferometer. Comparison of single dish CO data with B and V photometry is used to study the star formation efficiencies in gas-rich and gas-poor regions.
Authors
Wilson CD
Book title
Submillimetre Astronomy
Series
Astrophysics and Space Science Library
Volume
158
Pagination
pp. 161-162
Publisher
Springer Nature
Publication Date
1990
DOI
10.1007/978-94-015-6850-0_57