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Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades

Abstract:

The most powerful tests of stellar models come from the brightest stars in the sky, for which complementary techniques, such as astrometry, asteroseismology, spectroscopy, and interferometry can be combined. The K2 Mission is providing a unique opportunity to obtain high-precision photometric time series for bright stars along the ecliptic. However, bright targets require a large number of pixels to capture the entirety of the stellar flux, and bandwidth restrictions limit the number and brig...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.1093/mnras/stx1050

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
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Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
471
Issue:
3
Pages:
2882-2901
Publication date:
2017-08-11
Acceptance date:
2017-04-28
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:724356
URN:
uri:12ea5d7d-5a6a-46d9-b7f1-501e556f4ee4
UUID:
uuid:12ea5d7d-5a6a-46d9-b7f1-501e556f4ee4
Local pid:
pubs:724356
Paper number:
3

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