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Full Phase Coverage of BY Dra with the VLA
Published online by Cambridge University Press: 12 April 2016
Abstract
We have obtained 21 ~one-hour observations of the prototypical spotted star, BY Dra, with the VLA. These data are sufficiently well spaced in time to allow for complete rotational and orbital phase coverage; the resultant radio light curves are compared to their optical counterpart. We also plot the emission versus time without phase-folding, in order to search for longer periods of activity. Splitting the data into smaller (three minute) time bins allows for the determination of the normalized amplitude distribution of the flux; we compare this with known stellar optical and X-ray flare distributions.
- Type
- Part IV Stellar activity
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- Copyright © Springer-Verlag 1991