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  2. Wolfgang Kundt - Wikipedia

    en.wikipedia.org/wiki/Wolfgang_Kundt

    Download as PDF; Printable version; ... (2nd edition: Astrophysics. A New Approach. ebenda 2005, ... An Introduction to Current Research.

  3. Andrew R. Liddle - Wikipedia

    en.wikipedia.org/wiki/Andrew_R._Liddle

    Andrew R. Liddle FRSE (born 9 June 1965) is a professor of astrophysics at the University of Lisbon. [1] From 2018 to 2020 he was a Visiting Fellow at the University of Waterloo. [2] From 2013 to 2017 he was Professor of astrophysics at the Royal Observatory Edinburgh. [2] Publications include books and over 260 papers.

  4. Gravitational collapse - Wikipedia

    en.wikipedia.org/wiki/Gravitational_collapse

    Download as PDF; Printable version; ... with a slight dusting of free electrons and protons mixed in. ... An Introduction to Modern Astrophysics (2nd ed.).

  5. Astrophysics for People in a Hurry - Wikipedia

    en.wikipedia.org/wiki/Astrophysics_for_People_in...

    Neil deGrasse Tyson's Astrophysics for People in a Hurry is a popular introduction to the main concepts and issues of modern astrophysics.The author explains the origin and structure of the Universe, the force of gravity, light, dark matter and dark energy, about our place in the Cosmos and how we try to understand its laws.

  6. Astrophysical fluid dynamics - Wikipedia

    en.wikipedia.org/wiki/Astrophysical_fluid_dynamics

    Astrophysical fluid dynamics is a branch of modern astronomy which deals with the motion of fluids in outer space using fluid mechanics, such as those that make up the Sun and other stars. [1] The subject covers the fundamentals of fluid mechanics using various equations , such as continuity equations , the Navier–Stokes equations , and Euler ...

  7. Great Debate (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Great_Debate_(astronomy)

    Download as PDF; Printable version; In other projects Wikidata item; Appearance. ... An Introduction to Modern Astrophysics (2nd ed.). Cambridge University Press.

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  9. Kelvin–Helmholtz mechanism - Wikipedia

    en.wikipedia.org/wiki/Kelvin–Helmholtz_mechanism

    The Kelvin–Helmholtz mechanism is an astronomical process that occurs when the surface of a star or a planet cools. The cooling causes the internal pressure to drop, and the star or planet shrinks as a result.

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