@inproceedings{35504c1e35704921bae9908a4a0cf200,
title = "Non-radial modes in AGB stars",
abstract = "The success of asteroseismology in characterising G-K giants has motivated the extension of the same techniques to stars after the central He-burning and M-giants. The latter have been usually studied only as radial pulsators; the presence, however, of fine-structure in the period-luminosity diagram of red variables in the Magellanic Clouds could result from the presence of non-radial oscillations, offering the potential of observational indexes based on non-radial oscillations also for luminous red giants. We present here the results of a first approach aiming to identify the origin of the sub-ridges in the sequence A of the LMC red variables.",
author = "Josefina Montalb{\'a}n and Michele Trabucchi and Paola Marigo and Wood, {Peter R.} and Giada Pastorelli",
note = "Publisher Copyright: {\textcopyright} 2017 The Authors, published by EDP Sciences.; 22nd Los Alamos Stellar Pulsation Conference Series Meeting 2016 ; Conference date: 28-11-2016 Through 02-12-2016",
year = "2017",
month = sep,
day = "8",
doi = "10.1051/epjconf/201715206008",
language = "English",
series = "EPJ Web of Conferences",
publisher = "EDP Sciences",
editor = "Wolfgang Gieren and Marcio Catelan and Wolfgang Gieren and Marcio Catelan",
booktitle = "Wide-Field Variability Surveys",
address = "France",
}