Two large amplitude slowly pulsating hot subdwarf stars

dc.contributor.author	Koen, Chris
dc.date.accessioned	2013-10-16T19:56:03Z
dc.date.available	2013-10-16T19:56:03Z
dc.date.issued	2011
dc.identifier.citation	Koen, C. (2011). Two large amplitude slowly pulsating hot subdwarf stars. Monthly Notices of the Royal Astronomical Society, 415(4): 3042–3048	en_US
dc.identifier.issn	0035-8711
dc.identifier.uri	http://hdl.handle.net/10566/766
dc.description.abstract	The discovery observations of two new slowly pulsating subdwarf B stars (V1093 Her stars), BPS CS22890−74 and PB 7032, are presented. Both stars are highly multiperiodic, and have – for V1093 Her stars – large amplitudes. Published descriptions of the (wavelength) spectra of the stars conflict, but new spectra show that both are sdB stars with effective temperatures below 30 000 K. BPS CS22890−74 has a cool companion.	en_US
dc.language.iso	en	en_US
dc.publisher	Oxford University Press	en_US
dc.rights	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.1365-2966.2011.18929.x
dc.subject	Stars: individual: BPS CS22890−74	en_US
dc.subject	Stars: individual: PB 7032	en_US
dc.subject	Stars: oscillations: subdwarfs	en_US
dc.title	Two large amplitude 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