On possible explanations of pulsations in Maia stars
Solar and Stellar Astrophysics
2017-11-08 v1
Abstract
The long-time photometric surveys in a few young open clusters allowed to identify the light variability in stars located on the HR diagram between the well defined Scuti variables and Slowly Pulsating B-type stars. Several objects of this type were suggested also from the analysis of the Kepler data. Assuming the pulsational origin of this variability, we try to explain the observed frequencies with pulsational models involving rotation and/or modification of the mean opacity profile.
Cite
@article{arxiv.1701.00937,
title = {On possible explanations of pulsations in Maia stars},
author = {Jadwiga Daszynska-Daszkiewicz and Przemyslaw Walczak and Alexey Pamyatnykh},
journal= {arXiv preprint arXiv:1701.00937},
year = {2017}
}
Comments
proceedings of the Joint TASC2 - KASC9 Workshop - SPACEINN - HELAS8 Conference "Seismology of the Sun and the Distant Stars 2016", to be published by the EPJ Web of Conferences