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What is Molecular Clouds in M 33: Properties & Rotation about?
This study investigates the properties and rotation of 566 molecular clouds in the galaxy M 33, focusing on their star-forming characteristics and size-linewidth relations. The findings indicate that the linewidths of these clouds decrease with galactocentric distance and that the mass spectrum of non-star-forming clouds is steeper than that of star-forming clouds. Additionally, the research reveals weak velocity gradients in the clouds, suggesting low angular momentum and minimal influence on the evolution
- Author
- ljliu.astro
- Language
- EN