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2017MNRAS.471.2882W - Mon. Not. R. Astron. Soc., 471, 2882-2901 (2017/November-1)
Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades.
WHITE T.R., POPE B.J.S., ANTOCI V., PAPICS P.I., AERTS C., GIES D.R., GORDON K., HUBER D., SCHAEFER G.H., AIGRAIN S., ALBRECHT S., BARCLAY T., BARENTSEN G., BECK P.G., BEDDING T.R., FREDSLUND ANDERSEN M., GRUNDAHL F., HOWELL S.B., IRELAND M.J., MURPHY S.J., NIELSEN M.B., SILVA AGUIRRE V. and TUTHILL P.G.
Abstract (from CDS):
Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): asteroseismology - techniques: photometric - stars: early type - stars: variables: general - open clusters and associations: individual: Pleiades - open clusters and associations: individual: Pleiades
Simbad objects: 44
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