A search for short time-scale JHK variability in ultracool dwarfs

被引:38
作者
Koen, C
Matsunaga, N
Menzies, J
机构
[1] S African Astron Observ, ZA-7935 Observatory, Cape, South Africa
[2] Univ Tokyo, Sch Sci, Inst Astron, Tokyo 1818588, Japan
关键词
stars; low-mass; brown dwarfs; stars : variables : other;
D O I
10.1111/j.1365-2966.2004.08208.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The results of continuous monitoring, with typical durations of 2-4 h, of 18 L and T dwarfs are presented. Measurements were made simultaneously in JHK(S), with a typical time resolution of about 10 min. Limits on the variability are well below 0.02 mag in all cases except for the faintest object. There are none the less a fewdwarfs in which we may have observed variability: the same patterns of very low-level activity seemed to be present in the data for more than one filter. Simultaneous frequency-domain analysis of the J, H and K-S data furthermore hints at a very short period (0.8-1.6 h) in a few objects. We also present a brief assessment of some of the variability test statistics that have been used in the field of ultracool dwarf variability.
引用
收藏
页码:466 / 476
页数:11
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