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Post Info TOPIC: Carina-Near Moving Group


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Posts: 131433
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Magnetic activity on AB Doradus
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Title: Magnetic activity on AB Doradus: Temporal evolution of starspots and differential rotation from 1988 to 1994
Authors: S.V. Jeffers (1,2), J.-F. Donati (1), A.Collier Cameron (2) (1 LATT, Observatoire Midi-Pyrenees) (2, University of St Andrews)

Surface brightness maps for the young K0 dwarf AB Doradus are reconstructed from archival data sets for epochs spanning 1988 to 1994. By using the signal-to-noise enhancement technique of Least-Squares Deconvolution, our results show a greatly increased resolution of spot features than obtained in previously published surface brightness reconstructions. These images show that for the exception of epoch 1988.96, the starspot distributions are dominated by a long-lived polar cap, and short-lived low to high latitude features. The fragmented polar cap at epoch 1988.96 could indicate a change in the nature of the dynamo in the star. For the first time we measure differential rotation for epochs with sufficient phase coverage (1992.05, 1993.89, 1994.87). These measurements show variations on a timescale of at least one year, with the strongest surface differential rotation ever measured for AB Dor occurring in 1994.86. In conjunction with previous investigations, our results represent the first long-term analysis of the temporal evolution of differential rotation on active stars.

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Posts: 131433
Date:
Carina-Near Moving Group
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Title: The Carina-Near Moving Group
Authors: B. Zuckerman, M.S. Bessell, Inseok Song, S. Kim

We identify a group of ~20 co-moving, mostly southern hemisphere, ~200 Myr old stars near Earth. Of the stars likely to be members of this Carina-Near Moving Group, in either its nucleus (~30 pc from Earth) or surrounding stream, all but 3 are plausible members of a multiple star system. The nucleus is (coincidentally) located quite close to the nucleus of the AB Doradus moving group notwithstanding that the two groups have substantially different ages and Galactic space motions, UVW.

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