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Pulsation models of O-rich and C-rich long period variables

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Date

2017-09-08

Authors

Trabucchi, Michele
Marigo, Paola
Montalbán, Josefina
Wood, Peter R.
Girardi, Léo

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Volume Title

Publisher

EDP Sciences

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Research Projects

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Abstract

The intrinsic variability of luminous red giants is an observable providing important information about stellar structure and evolution. Our aim is to provide a solid theoretical background to the wide amount of data coming from present and future variability surveys. We present here the first comparison between long period variables in the LMC (from OGLE-III) and our grid of pulsation models computed for a wide range of stellar parameters and input physics.

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Citation

URI

https://hdl.handle.net/1885/733799040

Collections

ANU Research Publications

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Type

Conference paper

Book Title

Wide-Field Variability Surveys: A 21st Century Perspective - 22nd Los Alamos Stellar Pulsation - Conference Series Meeting

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Publication

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DOI

10.1051/epjconf/201715206009

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