Division G WG Red Giants and Supergiants

Description

Quantitative understanding of red giants and red supergiants and their relation to stellar end products and galaxy evolution. This involves all input physics and related structural and evolutionary properties, such as mass-loss, internal mixing, nuclear reaction rates etc.

Note: Malpractice (or good practice) in the astronomical community can be reported anonymously to the IAU Division G Ombud.

Links:

• WG Annual Report (2024) - Red Giants and Supergiants
• WG Annual Report (2022) - Red Giants and Supergiants
• WG Annual Report (2021) - Red Giants and Supergiants
• WG Triennial Report (2018-2021) - Red Giants and Supergiants
• WG Annual Report (2019) - Red Giants and Supergiants
• WG Triennial Report (2015-2018) - Abundances in Red Giants
• Newsletter

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Regular Working Groups, unless re-established by the same procedure, such Working Groups cease to exist at the following General Assembly.

Re-established for the Triennium 2024-2027.

Working Group Members (17)

Under

Division G Stars and Stellar Physics