Evidence for rapid evolution of periodic variations in an ultracool dwarf

dc.contributor.author	Koen, Chris
dc.date.accessioned	2013-11-12T21:45:57Z
dc.date.available	2013-11-12T21:45:57Z
dc.date.issued	2006
dc.identifier.citation	Koen, C. (2006). Evidence for rapid evolution of periodic variations in an ultracool dwarf. Monthly Notices of the Royal Astronomical Society, 367: 1735–1738	en_US
dc.identifier.uri	http://hdl.handle.net/10566/799
dc.description.abstract	The results of three short photometric monitoring runs on the L0 dwarf 2MASS J06050196−2342270, during three consecutive nights, are presented. The observations show the persistent presence of a 2.4-h period, with an IC band amplitude which decreased from 27 to 11 mmag over the three nights. The amplitude in the RC band appeared to be substantially smaller than in the IC band.	en_US
dc.language.iso	en	en_US
dc.publisher	Oxford University Press	en_US
dc.rights	© 2006 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.1365-2966.2006.10059.x
dc.subject	Stars: low-mass, brown dwarfs	en_US
dc.subject	Stars: variables: other	en_US
dc.title	Evidence for rapid evolution of periodic variations in an ultracool dwarf	en_US
dc.type	Article	en_US
dc.privacy.showsubmitter	false
dc.status.ispeerreviewed	true
dc.description.accreditation	Web of Science	en_US