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

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dc.contributor.authorKoen, Chris
dc.date.accessioned2013-11-13T08:26:19Z
dc.date.available2013-11-13T08:26:19Z
dc.date.issued2005
dc.description.abstractThe 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.description.accreditationWeb of Scienceen_US
dc.identifier.citationKoen, C (2005). IC and RC band time-series observations of some bright ultracool dwarfs. Monthly Notices of the Royal Astronomical Society, 360: 1132–1142en_US
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/10566/805
dc.language.isoenen_US
dc.privacy.showsubmitterfalse
dc.publisherOxford University Pressen_US
dc.rightsCopyright 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.urihttp://dx.doi.org/10.1111/j.1365-2966.2005.09119.x
dc.status.ispeerreviewedtrue
dc.subjectStars: low-mass, brown dwarfsen_US
dc.subjectStars: variables: otheren_US
dc.titleIC and RC band time-series observations of some bright ultracool dwarfsen_US
dc.typeArticleen_US

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Research Articles (Statistics & Population Studies)
Prof. Chris Koen