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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
Abstract
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