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Pressure and Temperature Profiles in the Solar Nebula
Authors:John A Wood
Institution:(1) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
Abstract:Pressure and temperature profiles in several recent solar nebula models are reviewed. These parameters are important to cosmochemists because they determine the mineral assemblages that could form or exist in the nebula. This revised version was published online in June 2006 with corrections to the Cover Date.
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