| dc.contributor.author | Koen, Chris | |
| dc.contributor.author | Green, E.M. | |
| dc.date.accessioned | 2013-11-13T08:25:57Z | |
| dc.date.available | 2013-11-13T08:25:57Z | |
| dc.date.issued | 2010 | |
| dc.identifier.citation | Koen, C. & Green, E.M. (2010). PG 0907+123 and JL 194: slowly pulsating hot subdwarf stars. Monthly Notices of the Royal Astronomical Society, 406: 2701–2712 | en_US |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.uri | http://hdl.handle.net/10566/800 | |
| dc.description.abstract | Multicolour time-series photometry of two newly discovered slowly pulsating sdB stars
(V1093 Her stars, also known as PG 1716 stars) is described. Both stars are fairly bright
and appear, from the limited amount of data, to have rich pulsation spectra. Given that the
amplitudes of variation of both stars are also large compared to most PG 1716 stars, both are
good candidates for extensive follow-up observations. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.rights | © 2010 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.1365-2966.2010.16868.x | |
| dc.subject | Stars: individual: PG 0907+123 | en_US |
| dc.subject | Stars: individual: JL 194 | en_US |
| dc.subject | Stars: oscillations: subdwarfs | en_US |
| dc.subject | Stars: variables: general | en_US |
| dc.title | PG 0907+123 and JL 194: slowly pulsating hot subdwarf stars | en_US |
| dc.type | Article | en_US |
| dc.privacy.showsubmitter | false | |
| dc.status.ispeerreviewed | true | |
| dc.description.accreditation | Web of Science | en_US |
