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Single and Composite Hot Subdwarf Stars in the Light of 2MASS Photometry
Authors:MA Stark  Richard A Wade  GB Berriman
Institution:1. Armagh Observatory, Armagh, UK
2. American Museum of Natural History, New York, U.S.A
3. Max-Planck-Institut für Astronomie, Heidelberg, Germany
4. Max-Planck-Institut für Radioastronomie, Bonn, Germany
Abstract:We show that supersonic turbulence accelerates the transition ofan atomic cloud into a molecular cloud, quantified here through a demo model and 3D numerical simulations which explicitly includeatomic-molecular chemistry. Specific sites where amplifiedformation may be detectable are suggested.
Keywords:
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