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2. 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.

3. 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.

4. 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.

5. Vogt–Russell theorem - Wikipedia

   en.wikipedia.org/wiki/Vogt–Russell_theorem

   The Vogt–Russell theorem states that the structure of a star, in hydrostatic and thermal equilibrium with all energy derived from nuclear reactions, is uniquely determined by its mass and the distribution of chemical elements throughout its interior. [1]

6. Main sequence - Wikipedia

   en.wikipedia.org/wiki/Main_sequence

   Astrophysics I: Stars. Boston: Jones and Bartlett. Carroll, Bradley W. & Ostlie, Dale A. (2007). An Introduction to Modern Astrophysics. San Francisco: Pearson Education Addison-Wesley. ISBN 978-0-8053-0402-2. Chabrier, Gilles; Baraffe, Isabelle (2000). "Theory of Low-Mass Stars and Substellar Objects". Annual Review of Astronomy and Astrophysics.

7. 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.

8. AOL Mail

   mail.aol.com

   Get AOL Mail for FREE! Manage your email like never before with travel, photo & document views. Personalize your inbox with themes & tabs. You've Got Mail!

9. Stellar structure - Wikipedia

   en.wikipedia.org/wiki/Stellar_structure

   Download as PDF; Printable version; ... The mixing length theory contains two free parameters which must be ... (1998), Introductory Astronomy & Astrophysics (4th ed ...