Stellar Evolution during the Successive Nuclear Burning Phases

Autor: Claude Doom, C. De Loore
Rok vydání: 1992
Předmět:
Zdroj: Structure and Evolution of Single and Binary Stars ISBN: 9780792318446
DOI: 10.1007/978-94-011-2502-4_10
Popis: In the next chapters we will discuss the evolution of single stars. We may divide these stars into different groups according to their mass. Each group of stars has a different evolutionary history : After core hydrogen burning the low mass stars develop a helium core where the electrons are degenerate. This degeneracy is lifted by the helium flash.
Databáze: OpenAIRE