Abstract
We present a preliminary analysis of the data collected during the 1999/1 (XCOV17) Whole Earth Telescope (WET) campaign to observe the pulsating subdwarf B star PG 1336-018. Since PG1336-018 is an HW Vir type eclipsing binary, our hope is to use the known orbital period, assume a tidally locked system, and search for rotationally split modes. To this end, we can already report some success.
Original language | English |
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Pages (from-to) | 183-195 |
Number of pages | 13 |
Journal | Baltic Astronomy |
Volume | 9 |
Issue number | 2 |
DOIs | |
State | Published - 2000 |
Keywords
- Individual: PG 1336-018
- Oscillations
- Stars: subdwarf B