Stellar Evolution during the Successive Nuclear Burning Phases
Autor: | Claude Doom, C. De Loore |
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Rok vydání: | 1992 |
Předmět: |
Physics
Degenerate energy levels chemistry.chemical_element Astronomy Astrophysics::Cosmology and Extragalactic Astrophysics Helium flash Electron Stars chemistry Astrophysics::Solar and Stellar Astrophysics Physics::Atomic Physics Astrophysics::Earth and Planetary Astrophysics Low Mass Degeneracy (mathematics) Stellar evolution Astrophysics::Galaxy Astrophysics Helium |
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 |
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