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Mikkel Nørup Lund

Signatures of Magnetic Activity: On the Relation between Stellar Properties and p-mode Frequency Variations

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DOI

  • A. R.G. Santos, Space Science Institute
  • ,
  • T. L. Campante, University of Porto, Departamento de Física e Astronomia
  • ,
  • W. J. Chaplin, School of Physics and Astronomy, University of Birmingham, UK
  • ,
  • M. S. Cunha, University of Porto
  • ,
  • J. L. Van Saders, University of Hawaii at Manoa
  • ,
  • C. Karoff
  • T. S. Metcalfe
  • S. Mathur, Instituto de Astrofísica de Canarias, La Laguna University
  • ,
  • R. A. Garcia, Universite Paris-Saclay, Université Paris Diderot
  • ,
  • M. N. Lund
  • R. Kiefer, University of Warwick
  • ,
  • V. Silva Aguirre
  • G. R. Davies, School of Physics and Astronomy, University of Birmingham, UK
  • ,
  • R. Howe, School of Physics and Astronomy, University of Birmingham, UK
  • ,
  • Y. Elsworth, School of Physics and Astronomy, University of Birmingham, UK

In the Sun, the properties of acoustic modes are sensitive to changes in the magnetic activity. In particular, mode frequencies are observed to increase with increasing activity level. Thanks to CoRoT and Kepler, such variations have been found in other solar-type stars and encode information on the activity-related changes in their interiors. Thus, the unprecedented long-term Kepler photometric observations provide a unique opportunity to study stellar activity through asteroseismology. The goal of this work is to investigate the dependencies of the observed mode frequency variations on the stellar parameters and whether those are consistent with an activity-related origin. We select the solar-type oscillators with highest signal-to-noise ratio, in total, 75 targets. Using the temporal frequency variations determined in Santos et al., we study the relation between those variations and the fundamental stellar properties. We also compare the observed frequency shifts with chromospheric and photometric activity indexes, which are only available for a subset of the sample. We find that frequency shifts increase with increasing chromospheric activity, which is consistent with an activity-related origin of the observed frequency shifts. Frequency shifts are also found to increase with effective temperature, which is in agreement with the theoretical predictions for the activity-related frequency shifts by Metcalfe et al. Frequency shifts are largest for fast rotating and young stars, which is consistent with those being more active than slower rotators and older stars. Finally, we find evidence for frequency shifts increasing with stellar metallicity.

OriginalsprogEngelsk
Artikelnummer65
TidsskriftAstrophysical Journal
Vol/bind883
Nummer1
Antal sider9
ISSN0004-637X
DOI
StatusUdgivet - sep. 2019

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