Preliminary results from XCOV 17: PG 1336-018
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.
Individual: PG 1336-018, Oscillations, Stars: subdwarf B
Reed, M. D., D. Kilkenny, S. D. Kawaler, A. Mukadam, S. J. Kleinman, A. Nitta-Kleinman, J. L. Provencal et al. "Preliminary Results from XCOV 17: PG 1336-018." Baltic Astronomy 9, no. 2 (2000): 183-196.