Abstract
We present the first results of a spectroscopic survey of southern and equatorial Algol-type eclipsing binary systems with mass-accreting pulsating components (oEA stars) using the 2.4-m Thai National Telescope (TNT) and the 10-m South African Large Telescope (SALT). The survey aims to find orbital and binary parameters and to detect the high-degree non-radial pulsations (NRPs). We report the detection of high-degree NRPs in AS Eri, WYCet, VYHya, GQTrA, BDVir, and UWVir.
Original language | English |
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Pages (from-to) | 256-261 |
Number of pages | 6 |
Journal | Bulletin de la Societe Royale des Sciences de Liege |
Volume | 88 |
DOIs | |
Publication status | Published - 2019 |
Keywords
- Binaries
- Eclipsing
- OEA stars
- Oscillations
- Stars
ASJC Scopus subject areas
- Multidisciplinary