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:

Working Group Members (17)


Under

Division G Stars and Stellar Physics


Gioia Rau

NASA/Goddard Space Flight Center
Astrophysics
8800 Greenbelt Rd.
Greenbelt 20771
D.C.
United States

NCA adherence: United States

Last updated:
September 10, 2021

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