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Models of Collapsing Clouds and Star-Forming Regions as Analogs of the Solar Nebula
Published online by Cambridge University Press: 30 March 2016
Abstract
To fully understand the formation and the evolution of the Solar Nebula, the physical and chemical characteristics of the “pre-solar” cloud should be known. Here, I review recent findings on the study of starless and pre-stellar cores, pointing out the importance of molecular freeze out in the chemical and dynamical evolution of star forming regions.
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- I. Joint Discussions
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- Copyright © Astronomical Society of Pacific 2005