JL 82: a slowly pulsating hot subdwarf star in a close binary system

dc.contributor.author	Koen, Chris
dc.date.accessioned	2013-11-19T13:44:34Z
dc.date.available	2013-11-19T13:44:34Z
dc.date.issued	2009
dc.identifier.citation	Koen, C. (2009). JL 82: a slowly pulsating hot subdwarf star in a close binary system. Monthly Notices of the Royal Astronomical Society, 395(2): 979–984	en_US
dc.identifier.issn	0035-8711
dc.identifier.uri	http://hdl.handle.net/10566/839
dc.description.abstract	JL 82 is a known binary, consisting of an sdB star and a companion which is not directly observable in the optical. Photometric measurements reported in this paper show it to variable with both the binary period (∼0.75 d), as well as on much shorter time-scales. The shorter periods are ascribed to pulsation of the sdB star, making it a member of the PG 1716 class of pulsating stars.	en_US
dc.language.iso	en	en_US
dc.publisher	Oxford University Press	en_US
dc.rights	© 2009 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.1365-2966.2009.14588.x
dc.subject	Binaries: close	en_US
dc.subject	Stars: individual: JL 82	en_US
dc.subject	Stars: oscillations	en_US
dc.subject	Subdwarfs	en_US
dc.subject	Stars: variables: other	en_US
dc.title	JL 82: a slowly pulsating hot subdwarf star in a close binary system	en_US
dc.type	Article	en_US
dc.privacy.showsubmitter	false
dc.status.ispeerreviewed	true