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https://hdl.handle.net/2183/48659 Preliminary Results from XCOV 17: PG 1336-018
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Reed, M.D.
Kilkenny, D.
Kawaler, S.D.
Mukadam, A.
Kleinman, S.J.
Nitta-Kleinman, A
Provencal, J.L.
Watson, T.
Sullivan, D.
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Reed, M., Kilkenny, D., Kawaler, S., Mukadam, A., Kleinman, S., Nitta-Kleinman, A., Provencal, J., Watson, T., Sullivan, D., Sullivan, T., Shobbrook, B., Jiang, X., Ashoka, B., Seetha, S., Leibowitz, E., Ibbetson, P., Mendelson, H., Meistas, E., Kalytis, R., Alisauskas, D., O'Donoghue, D., Martinez, P., Wyk, F., Stobie, R., Marang, F., Zola, S., Krzesinski, J., Ogloza, W., Mosaklik, P., Silvotti, R., Piccioni, A., Vauclair, G., Dolez, N., Rene-Fremy, J., Chevreton, M., Ulla, A., Dreizler, S., Schuh, S., Deetjen, J., Solheim, J., Perez, J., Suarez, O., Manteiga, M., Burleigh, M., Barstow, M., Kepler, S., Kanaan, A., Giovannini, O., Metcalfe, T. & Ostensen, R. (2000). Preliminary Results from XCOV 17: PG 1336-018. Open Astronomy, 9(2), 183-196. https://doi.org/10.1515/astro-2000-0202
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Abstract
[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 PG 1336-018 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.
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