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Density Wave Related Molecular Cloud Spiral Arms in M51
Published online by Cambridge University Press: 04 August 2017
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Results from a continuing study (Figure 1a) of the CO (J = 1-0) distribution in M51 are presented. The angular resolution (beam size 33″ = 1.5 kpc) and pointing stability (better than 4″) of the Onsala 20-m telescope have extracted a number of new features of the molecular cloud distribution and kinematics of M51 [1,2]:
- Type
- II. Large Scale Processes of Star Formation
- Information
- Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 535 - 538
- Copyright
- Copyright © Reidel 1987
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