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Estimating the p-mode frequencies of the solar twin 18 Scorpii

Identifieur interne : 005C83 ( Main/Exploration ); précédent : 005C82; suivant : 005C84

Estimating the p-mode frequencies of the solar twin 18 Scorpii

Auteurs : M. Bazot [Portugal] ; T. L. Campante [Portugal] ; W. J. Chaplin [Royaume-Uni] ; H. Carfantan [France] ; T. R. Bedding [Australie] ; X. Dumusque [Portugal, Suisse] ; A.-M. Broomhall [Royaume-Uni] ; P. Petit [France] ; S. Theado [France] ; V. Van Grootel [France] ; T. Arentoft [Danemark] ; M. Castro [Brésil] ; J. Christensen-Dalsgaard [Danemark] ; J.-D. Jr Do Nascimento [Brésil] ; B. Dintrans [France] ; H. Kjeldsen [Danemark] ; M. J. P. F. G. Monteiro [Portugal] ; N. C. Santos [Portugal] ; S. Sousa [Portugal] ; S. Vauclair [France]

Source :

RBID : Pascal:12-0411767

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English descriptors

Abstract

Solar twins have been a focus of attention for more than a decade, because their structure is extremely close to that of the Sun. Today, thanks to high-precision spectrometers, it is possible to use asteroseismology to probe their interiors. Our goal is to use time series obtained from the HARPS spectrometer to extract the oscillation frequencies of 18 Sco, the brightest solar twin. We used the tools of spectral analysis to estimate these quantities. We estimate 52 frequencies using an MCMC algorithm. After examination of their probability densities and comparison with results from direct MAP optimization, we obtain a minimal set of 21 reliable modes. The identification of each pulsation mode is straightforwardly accomplished by comparing to the well-established solar pulsation modes. We also derived some basic seismic indicators using these values. These results offer a good basis to start a detailed seismic analysis of 18 Sco using stellar models.


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<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
<imprint>
<date when="2012">2012</date>
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<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
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<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Algorithms</term>
<term>Astroseismology</term>
<term>Data analysis</term>
<term>Optimization</term>
<term>Oscillation frequency</term>
<term>Probability density</term>
<term>Radial velocity</term>
<term>Solar pulsations</term>
<term>Spectral analysis</term>
<term>Star models</term>
<term>Sun</term>
<term>Time series</term>
<term>p mode</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Mode p</term>
<term>Soleil</term>
<term>Astéroséismologie</term>
<term>Série temporelle</term>
<term>Fréquence oscillation</term>
<term>Analyse spectrale</term>
<term>Algorithme</term>
<term>Densité probabilité</term>
<term>Optimisation</term>
<term>Pulsation solaire</term>
<term>Modèle stellaire</term>
<term>Vitesse radiale</term>
<term>Analyse donnée</term>
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<div type="abstract" xml:lang="en">Solar twins have been a focus of attention for more than a decade, because their structure is extremely close to that of the Sun. Today, thanks to high-precision spectrometers, it is possible to use asteroseismology to probe their interiors. Our goal is to use time series obtained from the HARPS spectrometer to extract the oscillation frequencies of 18 Sco, the brightest solar twin. We used the tools of spectral analysis to estimate these quantities. We estimate 52 frequencies using an MCMC algorithm. After examination of their probability densities and comparison with results from direct MAP optimization, we obtain a minimal set of 21 reliable modes. The identification of each pulsation mode is straightforwardly accomplished by comparing to the well-established solar pulsation modes. We also derived some basic seismic indicators using these values. These results offer a good basis to start a detailed seismic analysis of 18 Sco using stellar models.</div>
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<li>Australie</li>
<li>Brésil</li>
<li>Danemark</li>
<li>France</li>
<li>Portugal</li>
<li>Royaume-Uni</li>
<li>Suisse</li>
</country>
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<li>Angleterre</li>
<li>Midi-Pyrénées</li>
<li>Midlands de l'Ouest</li>
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