Titlebook: An Introduction to the Evolution of Single and Binary Stars; Matthew Benacquista Textbook 2013 Springer Science+Business Media New York 20

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An Introduction to the Evolution of Single and Binary Stars978-1-4419-9991-7Series ISSN 2192-4791 Series E-ISSN 2192-4805

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,Europ?ische Priorit?t, 1974 bis 1981,e time exploring the envelopes of stars. We will revisit the energy density and pressure due to radiation and discuss the consequences of local thermodynamic equilibrium. Finally, we will also look in more detail at the nature of absorption lines in stellar spectra.

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Die deutsch-tschechischen Europaregionenpencil balanced on its point is also in equilibrium, but it is not stable against small perturbations. We now need to consider when our equilibrium solutions are also stable against small perturbations. In so doing, we will encounter a number of potential instabilities that may have a significant effect in the structure and evolution of stars.

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