KPD 0629–0016, a slowly pulsating hot subdwarf star

dc.contributor.authorKoen, Chris
dc.contributor.authorGreen, E.M.
dc.date.accessioned2013-11-19T14:03:51Z
dc.date.available2013-11-19T14:03:51Z
dc.date.issued2007
dc.description.abstractThe results of nine CCD photometric observing runs on KPD 0629–0016 are presented. During six of the runs measurements were obtained alternately through B and V filters. Four periodicities, for which there is good agreement between the frequencies identified in the B and V data, were extracted: these lie in the range 46–81 min. A fifth lower frequency appears to be definitely present, but is very uncertain due to aliasing. The ratios of the mode amplitudes measured in B and V, and the phase differences between variations in the two colours, are compatible with pulsation theory.en_US
dc.identifier.citationKoen, C. & Green, E.M (2007). KPD 0629–0016, a slowly pulsating hot subdwarf star. Monthly Notices of the Royal Astronomical Society, 377(4): 1605–1609en_US
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/10566/841
dc.language.isoenen_US
dc.privacy.showsubmitterfalse
dc.publisherOxford University Pressen_US
dc.rights© 2007 copyright Oxford University Press. This file may be freely used for educational purposes, as long as it is not altered in any way. Acknowledgement of the authors and the source is required.
dc.source.urihttp://dx.doi.org/10.1111/j.1365-2966.2007.11716.x
dc.status.ispeerreviewedtrue
dc.subjectStars: individual: KPD 0629–0016en_US
dc.subjectStars: oscillationsen_US
dc.subjectSubdwarfsen_US
dc.subjectStars: variables: otheren_US
dc.titleKPD 0629–0016, a slowly pulsating hot subdwarf staren_US
dc.typeArticleen_US

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