No CrossRef data available.
Article contents
Mass-losing AGB Stars in the LMC
Published online by Cambridge University Press: 25 May 2016
Abstract
We show the results of an infrared study of a sample of heavily obscured AGB stars in the LMC. Both carbon-rich and oxygen-rich mass-losing AGB stars can be found at both high and low luminosities, but the percentage of carbon stars decreases with increasing luminosity. The optical depth of the circumstellar envelopes also decreases with increasing luminosity, while the mass-loss rates are (nearly) constant with luminosity. We also show tentative evidence for having found the first post-AGB stars in the LMC.
- Type
- Session III — Observed Spectra and Energy Distributions
- Information
- Symposium - International Astronomical Union , Volume 177: The Carbon Star Phenomenon , 2000 , pp. 145 - 151
- Copyright
- Copyright © Kluwer 2000