Relation of Observable Stellar Parameters to Mass-loss Rate of AGB Stars in the LMC

• Published in: The Astrophysical journal 2022-12, Vol.941 (1), p.44
• Main Authors: Prager, Henry A., Willson, Lee Anne, Marengo, Massimo, Creech-Eakman, Michelle J.
• Format: Article
• Language: English
• Subjects: ASTRONOMY AND ASTROPHYSICS; Astrophysics; Asymptotic giant branch stars; Carbon; Carbon stars; Evolved stars; Late-type giant stars; Low mass stars; Luminosity; M giant stars; Mira variable stars; Oxygen; Pulsating variable stars; Pulsation; Pulsation modes; Semi-regular variable stars; Stars; Stellar mass loss; Stellar pulsations
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/ac9e57

Using the data set of Riebel et al. for 6889 pulsating AGB stars in the LMC, we have derived formulae for mass-loss rate as a function of luminosity and pulsation period, or luminosity and mass, in three ways, for each of five subsets of data: fundamental-mode oxygen-rich stars, first-overtone-mode oxygen-rich stars, fundamental-mode carbon stars, first-overtone-mode carbon stars, and extreme carbon stars. Using the distribution of the stars in period versus luminosity and mass versus luminosity, we are able to derive a power-law fit to the dependence of mass-loss rate on those quantities. This results in formulae that reproduce observed mass-loss rates and are in general agreement with the expectation from mass-loss models that the mass-loss rate is highly sensitive to luminosity, mass, and pulsation period. In the process of carrying out this analysis we have found radius–mass–luminosity relations and examined pulsation–mass–radius relations using published evolutionary and pulsation models. These allow us to derive mass and radius from the observed quantities luminosity and pulsation period. We also derived new mass-loss rate versus color relations.