EPJ Web of Conferences
Volume 101, 2015The Space Photometry Revolution – CoRoT Symposium 3, Kepler KASC-7 Joint Meeting
|Number of page(s)||2|
|Section||Session 6 – Posters|
|Published online||23 September 2015|
Testing the νmax scaling relation
1 School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK.
2 Stellar Astrophysics Centre (SAC), Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark.
3 Department of Physics and Astronomy, Yale University, P.O. Box 208101, New Haven, CT, 06520, USA.
4 Instituto de Ciencias del Espacio (CSIC - IEEC), Facultad de Ciencies, Campus UAB, E-08193 Bellaterra, Spain.
a e-mail: firstname.lastname@example.org
Published online: 23 September 2015
Two key global seismic quantities are relevant to estimate the fundamental properties of a star: the frequency of maximum power (νmax) and the large frequency separation (Δν). The focus of this work is to test the νmax scaling relation in order to ascertain it’s level of accuracy. Here we report our results using artificial data and real Kepler data, based on a grid-modelling approach.
© Owned by the authors, published by EDP Sciences, 2015
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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