Scholarly Works

Studies of Star Forming Regions in M33

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

January 1, 1990

DOI

10.1007/978-94-015-6850-0_57

Associated Experts

Christine D Wilson

Professor, Faculty of Science

Labels

Fields of Research (FoR)

5109 Space Sciences 51 Physical Sciences

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