Testing the νmax scaling relation
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...
| Main Authors: | , , , , , |
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| Format: | Article |
| Language: | English |
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EDP Sciences
2015-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/201510106017 |
| _version_ | 1818716044663980032 |
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| author | Coelho H. R. Chaplin W. J. Basu S. Serenelli A. Miglio A. Reese D. |
| author_facet | Coelho H. R. Chaplin W. J. Basu S. Serenelli A. Miglio A. Reese D. |
| author_sort | Coelho H. R. |
| collection | DOAJ |
| description | 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. |
| first_indexed | 2024-12-17T19:13:00Z |
| format | Article |
| id | doaj.art-67338f81f2ec400cb704772a4fd5912f |
| institution | Directory Open Access Journal |
| issn | 2100-014X |
| language | English |
| last_indexed | 2024-12-17T19:13:00Z |
| publishDate | 2015-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| series | EPJ Web of Conferences |
| spelling | doaj.art-67338f81f2ec400cb704772a4fd5912f2022-12-21T21:35:48ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-011010601710.1051/epjconf/201510106017epjconf_sphr2014_06017Testing the νmax scaling relationCoelho H. R.Chaplin W. J.Basu S.0Serenelli A.1Miglio A.Reese D.Department of Physics and Astronomy, Yale UniversityInstituto de Ciencias del Espacio (CSIC - IEEC), Facultad de CienciesTwo 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.http://dx.doi.org/10.1051/epjconf/201510106017 |
| spellingShingle | Coelho H. R. Chaplin W. J. Basu S. Serenelli A. Miglio A. Reese D. Testing the νmax scaling relation EPJ Web of Conferences |
| title | Testing the νmax scaling relation |
| title_full | Testing the νmax scaling relation |
| title_fullStr | Testing the νmax scaling relation |
| title_full_unstemmed | Testing the νmax scaling relation |
| title_short | Testing the νmax scaling relation |
| title_sort | testing the νmax scaling relation |
| url | http://dx.doi.org/10.1051/epjconf/201510106017 |
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