Testing Asteroseismic Scaling Relations with Interferometry

The asteroseismic scaling relations for the frequency of maximum oscillation power, vmax, and the large frequency separation, Δν, provide an easy way to directly determine the masses and radii of stars with detected solar-like oscillations. With the vast amount of data available from the CoRoT and K...

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Main Authors: White T. R., Aguirre V. Silva, Boyajian T., Creevey O., Huber D., von Braun K., Bedding T. R., Elsworth Y., Hekker S., Stello D., Weiss A.
Format: Article
Language:English
Published: EDP Sciences 2015-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201510106068
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author White T. R.
Aguirre V. Silva
Boyajian T.
Creevey O.
Huber D.
von Braun K.
Bedding T. R.
Elsworth Y.
Hekker S.
Stello D.
Weiss A.
author_facet White T. R.
Aguirre V. Silva
Boyajian T.
Creevey O.
Huber D.
von Braun K.
Bedding T. R.
Elsworth Y.
Hekker S.
Stello D.
Weiss A.
author_sort White T. R.
collection DOAJ
description The asteroseismic scaling relations for the frequency of maximum oscillation power, vmax, and the large frequency separation, Δν, provide an easy way to directly determine the masses and radii of stars with detected solar-like oscillations. With the vast amount of data available from the CoRoT and Kepler missions, the convenience of the scaling relations has resulted in their wide-spread use. But how valid are the scaling relations when applied to red giants, which have a substantially different structure than the Sun? Verifying the scaling relations empirically requires independent measurements. We report on the current state and future prospects of interferometric tests of the scaling relations.
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spelling doaj.art-9bb129aa39034eb4942a1e82641338402022-12-21T21:35:47ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-011010606810.1051/epjconf/201510106068epjconf_sphr2014_06068Testing Asteroseismic Scaling Relations with InterferometryWhite T. R.0Aguirre V. Silva1Boyajian T.2Creevey O.3Huber D.von Braun K.4Bedding T. R.Elsworth Y.Hekker S.Stello D.Weiss A.5Institut für Astrophysik, Georg-August-Universität GöttingenStellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus UniversityDepartment of Astronomy, Yale UniversityInstitut d’Astrophysique Spatiale, Université Paris XI - CNRS (UMR8617)Max-Planck-Institute for Astronomy (MPIA), Konigstuhl 17Max-Planck-Institut für AstrophysikThe asteroseismic scaling relations for the frequency of maximum oscillation power, vmax, and the large frequency separation, Δν, provide an easy way to directly determine the masses and radii of stars with detected solar-like oscillations. With the vast amount of data available from the CoRoT and Kepler missions, the convenience of the scaling relations has resulted in their wide-spread use. But how valid are the scaling relations when applied to red giants, which have a substantially different structure than the Sun? Verifying the scaling relations empirically requires independent measurements. We report on the current state and future prospects of interferometric tests of the scaling relations.http://dx.doi.org/10.1051/epjconf/201510106068
spellingShingle White T. R.
Aguirre V. Silva
Boyajian T.
Creevey O.
Huber D.
von Braun K.
Bedding T. R.
Elsworth Y.
Hekker S.
Stello D.
Weiss A.
Testing Asteroseismic Scaling Relations with Interferometry
EPJ Web of Conferences
title Testing Asteroseismic Scaling Relations with Interferometry
title_full Testing Asteroseismic Scaling Relations with Interferometry
title_fullStr Testing Asteroseismic Scaling Relations with Interferometry
title_full_unstemmed Testing Asteroseismic Scaling Relations with Interferometry
title_short Testing Asteroseismic Scaling Relations with Interferometry
title_sort testing asteroseismic scaling relations with interferometry
url http://dx.doi.org/10.1051/epjconf/201510106068
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