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The Orion Nebula and the Sun as Probes of Galactic Chemical Evolution

Published online by Cambridge University Press:  04 August 2017

M. Peimbert
M. Peimbert*
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo, Postal 70-264, México 04510 D.F., MEXICO

Abstract

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The solar and the Orion nebula chemical abundances are discussed; their chemical compositions differ at least in the O/H, He/O and 12C/13C ratios. A review of processes that could be responsible for these differences is presented.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 111 - 121
Copyright
Copyright © Reidel 1987 

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