Paper:	Thermohaline Mixing and Isotopic Ratios in AGB Stars
Volume:	497, Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time
Page:	253
Authors:	Stancliffe, R. J.
Abstract:	I investigate the effects of thermohaline mixing on the isotopic ratios of asymptotic giant branch (AGB) stars. While thermohaline mixing has been shown to be an effective means of changing the surface composition of low-mass stars while they ascend the upper part of the giant branch, the effect of this mechanism on the AGB is almost negligible. The carbon isotopic ratio is barely affected during the earliest pulses, and as the 12C content increases due to third dredge-up this effect becomes seriously curtailed. This is because structural changes affect the relative locations of 3He-burning and the CNO cycle. While the isotopic ratios are barely affected by thermohaline mixing on the AGB, there is a substantial increase in the surface lithium abundance due to the action of this mechanism.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.036 seconds