NASA NTRS · 19660043492
Stellar evolution. V - The evolution of a 15 solar masses star from the main sequence through core helium burning.
Abstract
Evolution of 15 solar masses star from main sequence through helium core burning, comparing with evolution of less massive stars
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Iben, I., Jr.. 1966-02-01. Stellar evolution. V - The evolution of a 15 solar masses star from the main sequence through core helium burning.. https://ntrs.nasa.gov/citations/19660043492
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