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Book Synopsis

Understanding Stellar Evolution is based on a series of graduate-level courses taught at the University of Washington since 2004, and is written for physics and astronomy students and for anyone with a physics background who is interested in stars. It describes the structure and evolution of stars, with emphasis on the basic physical principles and the interplay between the different processes inside stars. Based on these principles, the evolution of low- and high-mass stars is explained from their formation to their death.

The physical effects described include nuclear reactions, energy transport, chemical mixing, pulsation, mass loss, and rotation. A short description of the evolution of interacting binaries is also included. Modern state-of-the-art evolution models that follow from these basic principles are compared with observations, providing a test for the understanding of the processes that occur inside stars. Where physical processes are complex, intuitive ex

Understanding Stellar Evolution

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Order before 4pm today for delivery by Tue 23 Dec 2025.

A Hardback by Emily M Levesque, Emily M Levesque

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    View other formats and editions of Understanding Stellar Evolution by Emily M Levesque

    Publisher: Institute of Physics Publishing
    Publication Date: 12/15/2017 12:00:00 AM
    ISBN13: 9780750312790, 978-0750312790
    ISBN10: 0750312793

    Description

    Book Synopsis

    Understanding Stellar Evolution is based on a series of graduate-level courses taught at the University of Washington since 2004, and is written for physics and astronomy students and for anyone with a physics background who is interested in stars. It describes the structure and evolution of stars, with emphasis on the basic physical principles and the interplay between the different processes inside stars. Based on these principles, the evolution of low- and high-mass stars is explained from their formation to their death.

    The physical effects described include nuclear reactions, energy transport, chemical mixing, pulsation, mass loss, and rotation. A short description of the evolution of interacting binaries is also included. Modern state-of-the-art evolution models that follow from these basic principles are compared with observations, providing a test for the understanding of the processes that occur inside stars. Where physical processes are complex, intuitive ex

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