KPD 0629–0016, a slowly pulsating hot subdwarf star
| dc.contributor.author | Koen, Chris | |
| dc.contributor.author | Green, E.M. | |
| dc.date.accessioned | 2013-11-19T14:03:51Z | |
| dc.date.available | 2013-11-19T14:03:51Z | |
| dc.date.issued | 2007 | |
| dc.description.abstract | The 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.citation | Koen, C. & Green, E.M (2007). KPD 0629–0016, a slowly pulsating hot subdwarf star. Monthly Notices of the Royal Astronomical Society, 377(4): 1605–1609 | en_US |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.uri | http://hdl.handle.net/10566/841 | |
| dc.language.iso | en | en_US |
| dc.privacy.showsubmitter | false | |
| dc.publisher | Oxford University Press | en_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.uri | http://dx.doi.org/10.1111/j.1365-2966.2007.11716.x | |
| dc.status.ispeerreviewed | true | |
| dc.subject | Stars: individual: KPD 0629–0016 | en_US |
| dc.subject | Stars: oscillations | en_US |
| dc.subject | Subdwarfs | en_US |
| dc.subject | Stars: variables: other | en_US |
| dc.title | KPD 0629–0016, a slowly pulsating hot subdwarf star | en_US |
| dc.type | Article | en_US |