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Round table discussion of session F: convection and rotation

Published online by Cambridge University Press:  01 August 2006

Ian W. Roxburgh
Ian W. Roxburgh*
Affiliation:
Astronomy Unit, Queen Mary, University of London, Mile End Road, London E14NS, UK. Observatoire de Paris, Place Jules Janssen, 92195 Meudon, France. email: i.w.roxburgh@qmul.ac.uk
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Abstract

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The Session F round table. and audience, considered the following questions:

  1. (i) what determines the differential rotation in stellar convective zones?

  2. (ii) If there really is a rapid inward increase in angular velocity in giants will it have significant effects in the late stages of stellar evolution?

  3. (iii) How effective is penetration above a convective core?

  4. (iv) Why is the solar core nearly uniformly rotating?

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S239: Convection in Astrophysics , August 2006 , pp. 443 - 445
Copyright
Copyright © International Astronomical Union 2007