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Optical variability of the ultracool dwarf TVLM 513-46546 : evidence for inhomogeneous dust clouds

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Littlefair, S. P., Dhillon, V. S., Marsh, T. R., Shahbaz, T., Martin, Eduardo L. and Copperwheat, C. M.. (2008) Optical variability of the ultracool dwarf TVLM 513-46546 : evidence for inhomogeneous dust clouds. Monthly Notices of the Royal Astronomical Society, Vol.391 (No.1). L88-L92. ISSN 0035-8711

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Official URL: http://dx.doi.org/10.1111/j.1745-3933.2008.00562.x

Abstract

We present multicolour photometry of the M8.5V ultracool dwarf 'pulsar' TVLM 513-46546 (hereafter TVLM 513) obtained with the triple-beam photometer ULTRACAM. Data were obtained simultaneously in the Sloan-g' and Sloan-i' bands. The previously reported sinusoidal variability, with a period of 2 h, is recovered here. However, the Sloan-g' and Sloan-i' light curves are anticorrelated, a fact which is incompatible with the currently proposed starspot explanation for the optical variability. The anticorrelated nature and relative amplitudes of the optical light curves are consistent with the effects of persistent dust clouds rotating on the surface of the star. In the absence of other plausible explanations for the optical variability of TVLM 513, it seems likely that dust cloud coverage combined with the rapid rotation of TVLM 513 is responsible for the optical variability in this object. However, crude modelling of a photosphere with partial dust cloud coverage shows that the anticorrelation can only be reproduced using cooler models than the literature temperature of TVLM 513. We suggest this discrepancy can be removed if more dust is present within the photosphere of TVLM 513 than theoretical model atmospheres predict, though a definitive statement on this matter will require the development of self-consistent models of partially dusty atmospheres.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science > Physics
Library of Congress Subject Headings (LCSH): Low mass stars, Brown dwarf stars, Cool stars
Journal or Publication Title: Monthly Notices of the Royal Astronomical Society
Publisher: Wiley-Blackwell Publishing, Inc
ISSN: 0035-8711
Date: 21 November 2008
Volume: Vol.391
Number: No.1
Number of Pages: 5
Page Range: L88-L92
Identification Number: 10.1111/j.1745-3933.2008.00562.x
Status: Peer Reviewed
Publication Status: Published
Funder: Particle Physics and Astronomy Research Council (Great Britain) (PPARC), Research Councils UK (RCUK), Science and Technology Facilities Council (Great Britain) (STFC)
Grant number: PP/D002370/1 (PPARC), PPA/G/S/2003/00058 (PPARC), ST/F002599/1 (STFC)
References: Allard F., Hauschildt P. H., Alexander D. R., Tamanai A., Schweitzer A., 2001, ApJ, 556, 357 Bailer-Jones C. A. L., 2002, A&A, 389, 963 Berger E. et al., 2001, Nat, 410, 338 Berger E. et al., 2008, ApJ, 673, 1080 Burgasser A. J., Putman M. E., 2005, ApJ, 626, 486 Burrows A., Sudarsky D., Hubeny I., 2006, ApJ, 640, 1063 Dahn C. C. et al., 2002, AJ, 124, 1170 Dhillon V. S. et al., 2007, MNRAS, 378, 825 Edelson R. A., Krolik J. H., 1988, ApJ, 333, 646 Gizis J. E., Monet D. G., Reid I. N., Kirkpatrick J. D., Liebert J., Williams R. J., 2000, AJ, 120, 1085 Gondoin P., 2008, A&A, 478, 883 Hallinan G., Antonova A., Doyle J. G., Bourke S., Brisken W. F., Golden A., 2006, ApJ, 653, 690 Hallinan G. et al., 2007, ApJ, 663, L25 Lane C. et al., 2007, ApJ, 668, L163 Littlefair S. P., Dhillon V. S., Marsh T. R., Shahbaz T., Mart´ın E. L., 2006, MNRAS, 370, 1208 Mohanty S., Basri G., 2003, ApJ, 583, 451 Mohanty S., Basri G., Shu F., Allard F., Chabrier G., 2002, ApJ, 571, 469 Rockenfeller B., Bailer-Jones C. A. L., Mundt R., 2006, A&A, 448, 1111 West A. A. et al., 2004, AJ, 128, 426
URI: http://wrap.warwick.ac.uk/id/eprint/28862

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