NASA NTRS · 19660043490
Stellar evolution. III - The evolution of a 5 solar masses star from the main sequence through core helium burning.
Abstract
Evolution of 5 solar masses star model from main sequence through core helium burning compared to 3 solar masses model, noting Hertzsprung-Russell diagram
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Iben, I., Jr.. 1966-02-01. Stellar evolution. III - The evolution of a 5 solar masses star from the main sequence through core helium burning.. https://ntrs.nasa.gov/citations/19660043490
Cite the original work for its findings. Save a collection to share your selection of sources.