IC and RC band time-series observations of some bright ultracool dwarfs

dc.contributor.author	Koen, Chris
dc.date.accessioned	2013-11-13T08:26:19Z
dc.date.available	2013-11-13T08:26:19Z
dc.date.issued	2005
dc.identifier.citation	Koen, C (2005). IC and RC band time-series observations of some bright ultracool dwarfs. Monthly Notices of the Royal Astronomical Society, 360: 1132–1142	en_US
dc.identifier.issn	0035-8711
dc.identifier.uri	http://hdl.handle.net/10566/805
dc.description.abstract	The results of more than 100 h of CCD photometric monitoring of 10 L dwarfs and two T dwarfs are presented. Reasonable evidence is shown for IC band variability in DENIS 0255−4700, DENIS 1705−0516 and 2M 2104−1037. Substantial brightening of the T dwarf binary Indi Bab was observed over the course of 3.6 h; it is unlikely that this could have been caused by surface spots. No unequivocal variability could be detected in the RC band.	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.1365-2966.2005.09119.x
dc.subject	Stars: low-mass, brown dwarfs	en_US
dc.subject	Stars: variables: other	en_US
dc.title	IC and RC band time-series observations of some bright ultracool dwarfs	en_US
dc.type	Article	en_US
dc.privacy.showsubmitter	false
dc.status.ispeerreviewed	true
dc.description.accreditation	Web of Science	en_US