Preliminary Results from XCOV 17: PG 1336-018

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UDC.coleccionInvestigación
UDC.departamentoCiencias da Navegación e Enxeñaría Mariña
UDC.endPage195
UDC.grupoInvLaboratorio Interdisciplinar de Aplicacións da Intelixencia Artificial (LIA2)
UDC.issue2
UDC.journalTitleOpen Astronomy
UDC.startPage183
UDC.volume9
dc.contributor.authorManteiga, Minia
dc.contributor.authorReed, M.D.
dc.contributor.authorKilkenny, D.
dc.contributor.authorKawaler, S.D.
dc.contributor.authorMukadam, A.
dc.contributor.authorKleinman, S.J.
dc.contributor.authorNitta-Kleinman, A
dc.contributor.authorProvencal, J.L.
dc.contributor.authorWatson, T.
dc.contributor.authorSullivan, D.
dc.date.accessioned2026-06-25T16:40:15Z
dc.date.available2026-06-25T16:40:15Z
dc.date.issued2000-06-01
dc.description.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.
dc.description.sponsorshipAcknoledgments. Among the many supporters of the observations reported here, we would like to acknowledge support from the U.S. National Science Foundation through grant NSF-YI/AST 9257049 to Iowa State University, and support from UNESCO through the International Institute of Theoretical and Applied Physics at Iowa State. MDR would also like to thank Y. Oda and the McDonald Observatory TAC for a generous allocation of telescope time.
dc.description.sponsorshipEstados Unidos. National Science Foundation; NSF-YI/AST 9257049
dc.identifier.citationReed, 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
dc.identifier.doi10.1515/ASTRO-2000-0202
dc.identifier.urihttps://hdl.handle.net/2183/48659
dc.language.isoeng
dc.publisherDe Gruyter Brill
dc.relation.urihttps://doi.org/10.1515/ASTRO-2000-0202
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internationalen
dc.rights.accessRightsopen access
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subjectStars
dc.subjectSubdwarf B
dc.subjectOscillations
dc.subjectIndividual PG 1336-018
dc.titlePreliminary Results from XCOV 17: PG 1336-018
dc.typejournal article
dc.type.hasVersionVoR
dspace.entity.typePublication
relation.isAuthorOfPublicationac152b53-40d7-47ed-a5d2-036b0374adb7
relation.isAuthorOfPublication.latestForDiscoveryac152b53-40d7-47ed-a5d2-036b0374adb7

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