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Large-scale changes of the cloud coverage in the e Indi Ba,Bb system

Hitchcock, J A; Helling, Ch; Scholz, A; Hodosan, G; Dominik, M; Hundertmark, M; Jørgensen, U G; Longa-Peña, P; Sajadian, S; Skottfelt, J; Snodgrass, C; Bozza, V; Burgdorf, M J; Campbell-White, J; Figuera Jaimes, Roberto; Fujii, Y I; Haikala, L K; Henning, T; Hinse, T C; Lowry, S; Mancini, L; Rahvar, S; Rabus, M; Southworth, J; von Essen, C; Collaboration, The MiNDSTEp

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Authors

J A Hitchcock

Ch Helling

A Scholz

G Hodosan

M Dominik

M Hundertmark

U G Jørgensen

P Longa-Peña

S Sajadian

J Skottfelt

C Snodgrass

V Bozza

M J Burgdorf

J Campbell-White

Roberto Figuera Jaimes

Y I Fujii

L K Haikala

T Henning

T C Hinse

S Lowry

L Mancini

S Rahvar

M Rabus

C von Essen

The MiNDSTEp Collaboration



Abstract

We present the results of 14 nights of I-band photometric monitoring of the nearby brown dwarf binary, e Indi Ba,Bb. Observations were acquired over 2 months, and total close to 42 hours of coverage at a typically high cadence of 1.4 minutes. At a separation of just 0.7?, we do not resolve the individual components, and so effectively treat the binary as if it were a single object. However, e Indi Ba (spectral type T1) is the brightest known T-type brown dwarf, and is expected to dominate the photometric signal. We typically find no strong variability associated with the target during each individual night of observing, but see significant changes in mean brightness - by as much as 0.10 magnitudes - over the 2 months of the campaign. This strong variation is apparent on a timescale of at least 2 days. We detect no clear periodic signature, which suggests we may be observing the T1 brown dwarf almost pole-on, and the days-long variability in mean brightness is caused by changes in the large-scale structure of the cloud coverage. Dynamic clouds will very likely produce lightning, and complementary high cadence V-band and Ha images were acquired to search for the emission signatures associated with stochastic ‘strikes’. We report no positive detections for the target in either of these passbands.

Citation

Hitchcock, J. A., Helling, C., Scholz, A., Hodosan, G., Dominik, M., Hundertmark, M., …Collaboration, T. M. (2020). Large-scale changes of the cloud coverage in the e Indi Ba,Bb system. Monthly Notices of the Royal Astronomical Society, 495(4), 3881-3899. https://doi.org/10.1093/mnras/staa1344

Journal Article Type Article
Acceptance Date May 6, 2020
Online Publication Date May 18, 2020
Publication Date 2020-07
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 495
Issue 4
Pages 3881-3899
DOI https://doi.org/10.1093/mnras/staa1344
Keywords techniques: photometric, brown dwarfs, stars: individual: ? Indi Ba and Bb
Publisher URL https://doi.org/10.1093/mnras/staa1344

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