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  • PHYS 232

    • Stellar Structure and Evolution . PHYS 232

    Physics of stellar structure, equations of state and heat transport. Birth of stars and physics of brown dwarfs. Thermonuclear burning and main sequence stellar structure. Evolution of stars and mass loss. Origin, physical structure, and cooling of compact objects.

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    No Prerequisites

    4

    Units

    Optional

    Grading

    1, 2, 3

    Passtime

    None

    Level Limit

    Letters and science

    College
    Instructors
    BILDSTEN L
    No info found
    Lecture
    PHELP2524
    M W
    09:30 AM - 10:45 AM
    3 / 50
    Enrollment Trends
    Grading Trends (7)
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    PHYS 232 Bildsten L Fall 2023 Total: 12
    PHYS 232 Bildsten L Spring 2022 Total: 14
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