1981•Unpublished venueRequires access

Grids of evolutionary models for the upper part of the HR diagram. Mass loss and the turning of some red supergiants into WR stars.

A. Maeder

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Key concepts: Physics, Supergiant, Astrophysics, Hertzsprung–Russell diagram, Red supergiant, Diagram, Stars, Stellar evolution

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Grids of evolutionary models for the upper part of the HR diagram. Mass loss and the turning of some red supergiants into WR stars. — Research Paper | ScholarLens