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Dynamics of Giant Molecular Clouds in the Density Wave Potential
Published online by Cambridge University Press: 04 August 2017
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We performed an N-body simulation of a system of gravitating particles modeling the system of stable Giant Molecular Clouds (GMCs) in the background density wave potential. The system of gravitating GMCs forms shocks in the spiral potential well, and shows a prominent spiral structure.
- Type
- II. Large Scale Processes of Star Formation
- Information
- Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 539 - 541
- Copyright
- Copyright © Reidel 1987