Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1644
Title: Observational evidence of optical variability in L dwarfs
Authors: Maiti, M
Keywords: stars: low-mass
brown dwarfs
stars: rotation
stars: variables
Issue Date: Apr-2007
Publisher: The American Astronomical Society
Citation: Astronomical Journal, Vol. 133, pp. 1633 - 1644
Abstract: The results of quasi-simultaneous continuous monitoring of six L dwarfs in the R and I bands are presented. A careful analysis of the data shows that the object 2MASSW J0036+1821 is variable in the I and R bands. The amplitudes of our variable object were found to be 0.010 in the I band and 0.030 in the R band. Interestingly, while 2MASSW J0036+1821 was variable in the I band, it remained nonvariable in the R band, and vice versa. As most of the previous variability search programs of L dwarfs were carried out in the I band, this is the first evidence of this type of strange phenomena. The time evolution and rapid formation of dust on a macroscopic scale can plausibly produce this type of nonperiodic random variability
URI: http://hdl.handle.net/2248/1644
Appears in Collections:IIAP Publications
Publications based on data from IAO, Hanle

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