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

T. R. White, B. J.S. Pope, V. Antoci, P. I. Pápics, C. Aerts, D. R. Gies, K. Gordon, D. Huber, G. H. Schaefer, S. Aigrain, S. Albrecht, T. Barclay, G. Barentsen, P. G. Beck, T. R. Bedding, M. Fredslund Andersen, F. Grundahl, S. B. Howell, M. J. Ireland, S. J. MurphyMartin Bo Nielsen, V. Silva Aguirre, P. G. Tuthill

Research output: Contribution to journalArticle

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 CCD saturation, as well as restrictions on data storage and bandwidth, limit the number and brightness of stars that can be observed. To overcome this, we have developed a new photometric technique, which we call halo photometry, to observe very bright stars using a limited number of pixels. Halo photometry is simple, fast and does not require extensive pixel allocation, and will allow us to use K2 and other photometric missions, such as TESS, to observe very bright stars for asteroseismology and to search for transiting exoplanets. We apply this method to the seven brightest stars in the Pleiades open cluster. Each star exhibits variability; six of the stars show what aremost likely slowly pulsating B-star pulsations, with amplitudes ranging from 20 to 2000 ppm. For the star Maia, we demonstrate the utility of combining K2 photometry with spectroscopy and interferometry to show that it is not a 'Maia variable', and to establish that its variability is caused by rotational modulation of a large chemical spot on a 10 d time-scale.

Original languageEnglish (US)
Pages (from-to)2882-2901
Number of pages20
JournalMonthly Notices of the Royal Astronomical Society
Volume471
Issue number3
DOIs
StatePublished - Jan 1 2017

Fingerprint

pixel
interferometry
stars
spectroscopy
photometry
asteroseismology
pixels
saturation
time series
timescale
halos
Pleiades
ecliptic
B stars
stellar models
astrometry
open clusters
extrasolar planets
data storage
sky

Keywords

  • Asteroseismology
  • Open clusters and associations: individual: Pleiades
  • Stars: early type
  • Stars: variables: general
  • Techniques: photometric

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

White, T. R., Pope, B. J. S., Antoci, V., Pápics, P. I., Aerts, C., Gies, D. R., ... Tuthill, P. G. (2017). Beyond the Kepler/K2 bright limit: Variability in the seven brightest members of the Pleiades. Monthly Notices of the Royal Astronomical Society, 471(3), 2882-2901. https://doi.org/10.1093/mnras/stx1050

Beyond the Kepler/K2 bright limit : Variability in the seven brightest members of the Pleiades. / White, T. R.; Pope, B. J.S.; Antoci, V.; Pápics, 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, Martin Bo; Silva Aguirre, V.; Tuthill, P. G.

In: Monthly Notices of the Royal Astronomical Society, Vol. 471, No. 3, 01.01.2017, p. 2882-2901.

Research output: Contribution to journalArticle

White, TR, Pope, BJS, Antoci, V, Pápics, PI, Aerts, C, Gies, DR, Gordon, K, Huber, D, Schaefer, GH, Aigrain, S, Albrecht, S, Barclay, T, Barentsen, G, Beck, PG, Bedding, TR, Fredslund Andersen, M, Grundahl, F, Howell, SB, Ireland, MJ, Murphy, SJ, Nielsen, MB, Silva Aguirre, V & Tuthill, PG 2017, 'Beyond the Kepler/K2 bright limit: Variability in the seven brightest members of the Pleiades', Monthly Notices of the Royal Astronomical Society, vol. 471, no. 3, pp. 2882-2901. https://doi.org/10.1093/mnras/stx1050
White, T. R. ; Pope, B. J.S. ; Antoci, V. ; Pápics, 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, Martin Bo ; Silva Aguirre, V. ; Tuthill, P. G. / Beyond the Kepler/K2 bright limit : Variability in the seven brightest members of the Pleiades. In: Monthly Notices of the Royal Astronomical Society. 2017 ; Vol. 471, No. 3. pp. 2882-2901.
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AU - Pápics, P. I.

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AU - Bedding, T. R.

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AU - Grundahl, F.

AU - Howell, S. B.

AU - Ireland, M. J.

AU - Murphy, S. J.

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KW - Stars: variables: general

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