Division G WG Abundances in Red Giants

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.

Working Group Members (11)


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
Fax: +44 178 271 2378
Email: jtvanloonkeeleacuk
Personal website: http://www.astro.keele.ac.uk/~jacco
Organization website: http://www.astro.keele.ac.uk/

Last updated:
December 6, 2017

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