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  2. Martin Schwarzschild - Wikipedia

    en.wikipedia.org/wiki/Martin_Schwarzschild

    Spitzer died 10 days before Schwarzschild. Schwarzschild's work in the fields of stellar structure and stellar evolution led to improved understanding of pulsating stars, differential solar rotation, post-main sequence evolutionary tracks on the Hertzsprung-Russell diagram (including how stars become red giants), hydrogen shell sources , the ...

  3. Stellar evolution - Wikipedia

    en.wikipedia.org/wiki/Stellar_evolution

    Stellar evolution is the process by which a star changes over the course of its lifetime and how it can lead to the creation of a new star. Depending on the mass of the star, its lifetime can range from a few million years for the most massive to trillions of years for the least massive, which is considerably longer than the current age of the ...

  4. Ejnar Hertzsprung - Wikipedia

    en.wikipedia.org/wiki/Ejnar_Hertzsprung

    The so-called "Hertzsprung–Russell Diagram" has been used ever since as a classification system to explain stellar types and stellar evolution. He also discovered two asteroids, one of which is 1627 Ivar, an Amor asteroid. [5] His wife Henrietta (1881–1956) was a daughter of the Dutch astronomer Jacobus Kapteyn.

  5. Algol paradox - Wikipedia

    en.wikipedia.org/wiki/Algol_paradox

    In stellar astronomy, the Algol paradox is a paradoxical situation when elements of a binary star seem to evolve in discord with the established theories of stellar evolution. [1] A fundamental feature of these theories is that the rate of evolution of stars depends on their mass: The greater the mass, the faster this evolution, and the more ...

  6. Bill Paxton (computer scientist) - Wikipedia

    en.wikipedia.org/wiki/Bill_Paxton_(computer...

    In 1990 Paxton retired from Adobe Systems and became an unofficial scholar in residence at the Kavli Institute for Theoretical Physics (KITP) at the University of California, Santa Barbara, where he started working on the physics of stellar evolution. He is responsible for the EZ stellar evolution program and the creation of the open-source ...

  7. Subrahmanyan Chandrasekhar - Wikipedia

    en.wikipedia.org/wiki/Subrahmanyan_Chandrasekhar

    Subrahmanyan Chandrasekhar FRS (/ ˌ tʃ ə n d r ə ˈ ʃ eɪ k ər /; [3] 19 October 1910 – 21 August 1995) [4] was an Indian-American theoretical physicist who made significant contributions to the scientific knowledge about the structure of stars, stellar evolution and black holes.

  8. Symbiotic binary - Wikipedia

    en.wikipedia.org/wiki/Symbiotic_binary

    Symbiotic binaries are of particular interest to astronomers as they can be used to learn about stellar evolution. They are also vital in the study of stellar wind, ionized nebulae, and accretion because of the unique interstellar dynamics present within the system.

  9. Theoretical astronomy - Wikipedia

    en.wikipedia.org/wiki/Theoretical_astronomy

    motion of planets, satellites and binary stars, stellar structure and evolution, N-body motions in clusters of stars and galaxies, black holes, and the expanding universe. [ 1 ] The aim of astronomy is to understand the physics and chemistry from the laboratory that is behind cosmic events so as to enrich our understanding of the cosmos and of ...

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