| Issue |
EPJ Web Conf.
Volume 160, 2017
Seismology of the Sun and the Distant Stars 2016 – Using Today’s Successes to Prepare the Future – TASC2 & KASC9 Workshop – SPACEINN & HELAS8 Conference
|
|
|---|---|---|
| Article Number | 03013 | |
| Number of page(s) | 4 | |
| Section | Seismology: Stars Near and in The Main Sequence | |
| DOI | https://doi.org/10.1051/epjconf/201716003013 | |
| Published online | 27 October 2017 | |
https://doi.org/10.1051/epjconf/201716003013
On possible explanations of pulsations in Maia stars
1
Inytut Astronomiczny, Uniwersytet Wrocławski, ul. Kopernika 11, Wrocław, Poland
2
Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716, Warsaw, Poland
⋆ e-mail: daszynska@astro.uni.wroc.pl
Published online: 27 October 2017
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 δ 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.
© Owned by the authors, published by EDP Sciences, 2017
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