The AGB Newsletter invites contributions related to Asymptotic Giant Branch
stars; dealing with their structure, behaviour, evolution or mass loss, with
their impact on the dynamical and chemical evolution of galaxies or their use
as tracers of intermediate-age populations. To help understand AGB stars and
their roles in the galactic ecology, we also welcome contributions on all
associated phenomena such as post-AGB evolution, Planetary Nebulae, white
dwarf mass functions, AGB Manqué stars, relevant nuclear,
astrochemical and mineralogical processes, et cetera, as well as
contributions on first ascent Red Giant Branch stars and massive red
supergiants that are similar to AGB stars.
Contributions may include papers submitted or accepted for publication in
refereed journals or conference proceedings, thesis abstracts, conference or
job announcements, or other scientific communications. Please use the options
below or on the menu bar on the left hand side.
The editors: Jacco van Loon
(Keele University, UK), Ambra Nanni (Padova, Italy) and
(The University of Manchester, UK)
Next issue: 3 January 2017
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