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Preliminary results from XCOV 17: PG 1336-018

  • M. D. Reed*
  • , D. Kilkenny
  • , S. D. Kawaler
  • , A. Mukadam
  • , S. J. Kleinman
  • , A. Nitta-Kleinman
  • , J. L. Provencal
  • , T. Watson
  • , D. Sullivan
  • , T. Sullivan
  • , B. Shobbrook
  • , X. J. Jiang
  • , B. N. Ashoka
  • , S. Seetha
  • , E. Leibowitz
  • , P. Ibbetson
  • , H. Mendelson
  • , E. G. Meištas
  • , R. Kalytis
  • , D. Ališauskas
  • D. O'Donoghue, P. Martinez, F. Van Wyk, R. Stobie, F. Marang, S. Zola, J. Krzesinski, W. Ogloza, P. Mosaklik, R. Silvotti, A. Piccioni, G. Vauclair, N. Dolez, J. Rene-Fremy, M. Chevreton, A. Ulla, S. Dreizler, S. Schuh, J. Deetjen, J. E. Solheim, J. Perez, O. Suarez, M. Manteiga, M. Burleigh, M. Barstow, S. O. Kepler, A. Kanaan, O. Giovannini, T. Metcalfe, R. Østensen
*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

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 languageEnglish
Pages (from-to)183-195
Number of pages13
JournalBaltic Astronomy
Volume9
Issue number2
DOIs
StatePublished - 2000

Keywords

  • Individual: PG 1336-018
  • Oscillations
  • Stars: subdwarf B

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