AustralieFrV1, Main, Exploration, bibRecord, 007275

Ground‐based follow‐up in relation to Kepler asteroseismic investigation

Identifieur interne : 007275 ( Main/Exploration ); précédent : 007274; suivant : 007276

Ground‐based follow‐up in relation to Kepler asteroseismic investigation

Auteurs : K. Uytterhoeven [France] ; M. Briquet [Belgique] ; H. Bruntt [France] ; P. De Cat [Belgique] ; S. Frandsen [Danemark] ; J. Gutiérrez-Soto [Espagne] ; L. Kiss [Hongrie, Australie] ; D. W. Kurtz [Royaume-Uni] ; M. Marconi [Italie] ; J. Molenda- Akowicz [Pologne] ; R. Stensen [Belgique] ; S. Randall [Allemagne] ; J. Southworth [Royaume-Uni] ; R. Szab [Hongrie] ; R. Kasc Working Groups On Ground-Based Observations

Source :

Astronomische Nachrichten [ 0004-6337 ] ; 2010-12.

RBID : ISTEX:35199FE70668BC32A7BCA8450356DAF7E52A56F0

English descriptors

Abstract

The Kepler space mission, successfully launched in March 2009, is providing continuous and high‐precision photometry of thousands of stars simultaneously. The uninterrupted time‐series of stars of all known pulsation types are a precious source for asteroseismic studies. The Kepler data do not provide information on the physical parameters, such as T eff, log g, metallicity, and v sin i, which are crucial for successful asteroseismic modelling. Additional ground‐based time‐series data are needed to characterize mode parameters in several types of pulsating stars. Therefore, ground‐based multi‐colour photometry and mid/high‐resolution spectroscopy are needed to complement the space data. We present ground‐based activities within KASC on selected asteroseismic Kepler targets of several pulsation types (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

Url:

https://api.istex.fr/document/35199FE70668BC32A7BCA8450356DAF7E52A56F0/fulltext/pdf

DOI: 10.1002/asna.201011444

Affiliations:

Links toward previous steps (curation, corpus...)

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to stream Istex, to step Curation: 000982
to stream Istex, to step Checkpoint: 000B92
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Le document en format XML

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<front><div type="abstract" xml:lang="en">The Kepler space mission, successfully launched in March 2009, is providing continuous and high‐precision photometry of thousands of stars simultaneously. The uninterrupted time‐series of stars of all known pulsation types are a precious source for asteroseismic studies. The Kepler data do not provide information on the physical parameters, such as  T eff, log g, metallicity, and v sin i, which are crucial for successful asteroseismic modelling. Additional ground‐based time‐series data are needed to characterize mode parameters in several types of pulsating stars. Therefore, ground‐based multi‐colour photometry and mid/high‐resolution spectroscopy are needed to complement the space data. We present ground‐based activities within KASC on selected asteroseismic Kepler targets of several pulsation types (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)</div>
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Ground‐based follow‐up in relation to Kepler asteroseismic investigation

Ground‐based follow‐up in relation to Kepler asteroseismic investigation

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