AGB Newsletter

Asymptotic Giant Branch stars and related phenomena

Official publication of the
IAU Working Group on Abundances in Red Giants


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 Albert Zijlstra (The University of Manchester, UK)

Next issue: 1 November 2018

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