Multimode Cepheids in the Large Magellanic Cloud - challenges for theory
Solar and Stellar Astrophysics
2009-10-02 v1
Abstract
Data on multimode Cepheids from OGLE-III catalog of the LMC Cepheids are confronted with results from model calculations. Models whose radial mode periods are consistent with observation are not always in agreement with published evolutionary models. Nonradial mode interpretation is considered for the cases of unusual period ratios. The greatest challenge for stellar pulsation theory is explanation of double-mode pulsators with period ratios near 0.6.
Cite
@article{arxiv.0907.1417,
title = {Multimode Cepheids in the Large Magellanic Cloud - challenges for theory},
author = {W. A. Dziembowski and R. Smolec},
journal= {arXiv preprint arXiv:0907.1417},
year = {2009}
}
Comments
3 pages, 4 figures, Stellar Pulsation: Challenges for Theory and Observation, Santa Fe, NM, 31 May - 5 June, 2009