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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

Paola Caselli
Paola Caselli*
Affiliation:
INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 1-50125 Firenze, Italy

Abstract

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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.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 504 - 507
Copyright
Copyright © Astronomical Society of Pacific 2005

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