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  2. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture06.pdf
    17 Oct 2022: and the most probablespeed is v =. 2kT/m for a Maxwell-Botzmann distribution. In cooler stars, where pressure broadening is most important, collisionswith neutral hydrogen atoms are the main source of
  3. DRAFT VERSION MAY 24, 2022Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/hcrs22.pdf
    24 May 2022: Sasha Hinkley ,1 Aarynn L. Carter ,2 Shrishmoy Ray ,1 Andrew Skemer,2 Beth Biller,3 Elodie Choquet,4 Maxwell A.

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