publication . Article . Preprint . 2006

Mass loss on the Asymptotic Giant Branch

Albert A. Zijlstra;
Open Access
  • Published: 03 May 2006 Journal: Proceedings of the International Astronomical Union, volume 2, page 55 (issn: 1743-9213, eissn: 1743-9221, Copyright policy)
  • Publisher: Cambridge University Press (CUP)
Mass loss on the Asymptotic Giant Branch provides the origin of planetary nebulae. This paper reviews several relevant aspects of AGB evolution: pulsation properties, mass loss formalisms and time variable mass loss, evidence for asymmetries on the AGB, binarity, ISM interaction, and mass loss at low metallicity. There is growing evidence that mass loss on the AGB is already asymmetric, but with spherically symmetric velocity fields. The origin of the rings may be in pulsational instabilities causing mass-loss variations on time scales of centuries.
Persistent Identifiers
arXiv: Astrophysics::Solar and Stellar AstrophysicsAstrophysics::Galaxy Astrophysics
free text keywords: Astronomy and Astrophysics, Asymptotic giant branch, Time variable, Stellar mass loss, Astrophysics, Astronomy, Physics, Metallicity, Stellar mass, Planetary nebula
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