In this paper it is investigated whether molecular outflows can support the turbulence in molecular clouds against decay. In the momentum-driven regime of molecular flows the time scale of the replenishment of the fluctuations is longer than the dissipation time scale of pure hydrodynamical superson
On the origin of stellar aggregates in molecular clouds
β Scribed by V.G. Surdin
- Publisher
- John Wiley and Sons
- Year
- 1989
- Tongue
- English
- Weight
- 182 KB
- Volume
- 310
- Category
- Article
- ISSN
- 0004-6337
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