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

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

*Corresponding author for this work

    Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

    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.

    Original languageEnglish
    Title of host publicationWide-Field Variability Surveys
    Subtitle of host publicationA 21st Century Perspective - 22nd Los Alamos Stellar Pulsation - Conference Series Meeting
    EditorsWolfgang Gieren, Marcio Catelan, Wolfgang Gieren, Marcio Catelan
    PublisherEDP Sciences
    ISBN (Electronic)9782759890248
    DOIs
    Publication statusPublished - 8 Sept 2017
    Event22nd Los Alamos Stellar Pulsation Conference Series Meeting 2016 - San Pedro de Atacama, Chile
    Duration: 28 Nov 20162 Dec 2016

    Publication series

    NameEPJ Web of Conferences
    Volume152
    ISSN (Print)2101-6275
    ISSN (Electronic)2100-014X

    Conference

    Conference22nd Los Alamos Stellar Pulsation Conference Series Meeting 2016
    Country/TerritoryChile
    CitySan Pedro de Atacama
    Period28/11/162/12/16

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