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The effect of non-isothermality on the gravitational collapse of spherical clouds and the evolution of protostellar accretion
Authors:E. I. Vorobyov   Shantanu Basu
Affiliation:Department of Physics and Astronomy, University of Western Ontario, London, Ontario, N6A 3K7, Canada;Institute of Physics, Stachki 194, Rostov-on-Don, Russia
Abstract:
Keywords:hydrodynamics    stars: formation    ISM: clouds    dust, extinction    ISM: molecules
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