Division G WG Red Giants and Supergiants

Description

Quantitative understanding of abundances in red-giants This involves all input physics and related structural and evolutionary properties, such as mass-loss, internal mixing, nuclear reaction rates etc.

Links:

Working Group Members (8)


Under

Division G Stars and Stellar Physics


Jacco Th. van Loon

Keele University
Astrophysics Group
Lennard-Jones Laboratories
Staffordshire ST5 5BG
United Kingdom

Phone: +44 178 273 3331
Email: jtvanloonkeeleacuk
Personal website: http://www.astro.keele.ac.uk/~jacco
Organization website: http://www.astro.keele.ac.uk/

NCA adherence: United Kingdom

Last updated:
November 27, 2018

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