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The double-mode nature of the HADS star GSC 00144-03031 and the Petersen diagram of the class

Identifieur interne : 00A398 ( Main/Exploration ); précédent : 00A397; suivant : 00A399

The double-mode nature of the HADS star GSC 00144-03031 and the Petersen diagram of the class

Auteurs : E. Poretti [Italie] ; J. C. Suarez [Espagne] ; P. G. Niarchos [Grèce] ; K. D. Gazeas [Grèce] ; V. N. Manimanis [Grèce] ; P. Van Cauteren [Belgique, France] ; P. Lampens [Belgique] ; P. Wils [Belgique] ; R. Alonso [Espagne] ; P. J. Amado [Espagne, Chili] ; J. A. Belmonte [Espagne] ; N. D. Butterworth [Australie] ; M. Martignoni [France] ; S. Martin-Ruiz [Espagne] ; P. Moskalik [Pologne] ; C. W. Robertson [États-Unis]

Source :

RBID : Pascal:05-0406446

Descripteurs français

English descriptors

Abstract

The double-mode pulsation of GSC 00144-03031 has been detected when searching for COROT targets. A very large dataset composed of 4722 photometric measurements was collected at six observatories in Europe and America. There is no hint of the excitation of additional modes (down to 0.6 mmag) and therefore GSC 00144-03031 seems to be a pure double-mode pulsator, with a very short fundamental radial mode (P = 84 min). From uvbyss photometry and evolutionary tracks it appears to be a Pop. I star with M = 1.75 M◦., located in the middle of the instability strip, close to the Zero-Age Main Sequence. We also discovered other new double-mode pulsators in the databases of large-scale projects: OGLE BW2_V142, OGLE BW1_V207, ASAS3 094303-1707.3, ASAS3 000116-6037.0, NSVS 3234596 and NSVS 3324715. An observational Petersen diagram is presented and explained by means of new models. A common sequence connecting Pop. I stars from the shortest to the longest periods is proposed and the spreads in the period ratios are ascribed to different metallicities (at the shortest periods) and to different masses (at the longest ones).


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Le document en format XML

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<inist:fA14 i1="10">
<s2>24 Payne Street, Mt. Louisa, Townsville, Queensland 4814</s2>
<s3>AUS</s3>
<sZ>12 aut.</sZ>
</inist:fA14>
<country>Australie</country>
<wicri:noRegion>24 Payne Street, Mt. Louisa, Townsville, Queensland 4814</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Martignoni, M" sort="Martignoni, M" uniqKey="Martignoni M" first="M." last="Martignoni">M. Martignoni</name>
<affiliation wicri:level="1">
<inist:fA14 i1="05">
<s1>Groupe Européen d'Observations Stellaires (GEOS), 23 Parc de Levesville</s1>
<s2>28300 Bailleau l'Evëque</s2>
<s3>FRA</s3>
<sZ>6 aut.</sZ>
<sZ>13 aut.</sZ>
</inist:fA14>
<country>France</country>
<wicri:noRegion>28300 Bailleau l'Evëque</wicri:noRegion>
<wicri:noRegion>23 Parc de Levesville</wicri:noRegion>
<wicri:noRegion>28300 Bailleau l'Evëque</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Martin Ruiz, S" sort="Martin Ruiz, S" uniqKey="Martin Ruiz S" first="S." last="Martin-Ruiz">S. Martin-Ruiz</name>
<affiliation wicri:level="2">
<inist:fA14 i1="02">
<s1>Instituto de Astrofisica de Andalucía, C.S.I.C., Apdo. 3004</s1>
<s2>18080 Granada</s2>
<s3>ESP</s3>
<sZ>2 aut.</sZ>
<sZ>10 aut.</sZ>
<sZ>14 aut.</sZ>
</inist:fA14>
<country>Espagne</country>
<placeName>
<region nuts="2" type="communauté">Andalousie</region>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Moskalik, P" sort="Moskalik, P" uniqKey="Moskalik P" first="P." last="Moskalik">P. Moskalik</name>
<affiliation wicri:level="1">
<inist:fA14 i1="11">
<s1>Nicolaus Copernicus Astronomical Center, ul. Bartycka 18</s1>
<s2>00-716 Warsaw</s2>
<s3>POL</s3>
<sZ>15 aut.</sZ>
</inist:fA14>
<country>Pologne</country>
<wicri:noRegion>00-716 Warsaw</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Robertson, C W" sort="Robertson, C W" uniqKey="Robertson C" first="C. W." last="Robertson">C. W. Robertson</name>
<affiliation wicri:level="1">
<inist:fA14 i1="12">
<s1>SETEC Observatory</s1>
<s2>Goddard, KS</s2>
<s3>USA</s3>
<sZ>16 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>SETEC Observatory</wicri:noRegion>
</affiliation>
</author>
</analytic>
<series>
<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="2005">2005</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt>
<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>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Age</term>
<term>Data analysis</term>
<term>Excitation</term>
<term>Instability strip</term>
<term>M stars</term>
<term>Metallicity</term>
<term>Models</term>
<term>Photometry</term>
<term>p mode</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Excitation</term>
<term>Mode p</term>
<term>Photométrie</term>
<term>Etoile M</term>
<term>Bande instabilité</term>
<term>Age</term>
<term>Modèle</term>
<term>Métallicité</term>
<term>Analyse donnée</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">The double-mode pulsation of GSC 00144-03031 has been detected when searching for COROT targets. A very large dataset composed of 4722 photometric measurements was collected at six observatories in Europe and America. There is no hint of the excitation of additional modes (down to 0.6 mmag) and therefore GSC 00144-03031 seems to be a pure double-mode pulsator, with a very short fundamental radial mode (P = 84 min). From uvbyss photometry and evolutionary tracks it appears to be a Pop. I star with M = 1.75 M
<sub>◦.</sub>
, located in the middle of the instability strip, close to the Zero-Age Main Sequence. We also discovered other new double-mode pulsators in the databases of large-scale projects: OGLE BW2_V142, OGLE BW1_V207, ASAS3 094303-1707.3, ASAS3 000116-6037.0, NSVS 3234596 and NSVS 3324715. An observational Petersen diagram is presented and explained by means of new models. A common sequence connecting Pop. I stars from the shortest to the longest periods is proposed and the spreads in the period ratios are ascribed to different metallicities (at the shortest periods) and to different masses (at the longest ones).</div>
</front>
</TEI>
<affiliations>
<list>
<country>
<li>Australie</li>
<li>Belgique</li>
<li>Chili</li>
<li>Espagne</li>
<li>France</li>
<li>Grèce</li>
<li>Italie</li>
<li>Pologne</li>
<li>États-Unis</li>
</country>
<region>
<li>Andalousie</li>
<li>Attique (région)</li>
<li>Vienne (Autriche)</li>
</region>
<settlement>
<li>Athènes</li>
<li>Vienne (Autriche)</li>
</settlement>
</list>
<tree>
<country name="Italie">
<noRegion>
<name sortKey="Poretti, E" sort="Poretti, E" uniqKey="Poretti E" first="E." last="Poretti">E. Poretti</name>
</noRegion>
</country>
<country name="Espagne">
<region name="Andalousie">
<name sortKey="Suarez, J C" sort="Suarez, J C" uniqKey="Suarez J" first="J. C." last="Suarez">J. C. Suarez</name>
</region>
<name sortKey="Alonso, R" sort="Alonso, R" uniqKey="Alonso R" first="R." last="Alonso">R. Alonso</name>
<name sortKey="Amado, P J" sort="Amado, P J" uniqKey="Amado P" first="P. J." last="Amado">P. J. Amado</name>
<name sortKey="Belmonte, J A" sort="Belmonte, J A" uniqKey="Belmonte J" first="J. A." last="Belmonte">J. A. Belmonte</name>
<name sortKey="Martin Ruiz, S" sort="Martin Ruiz, S" uniqKey="Martin Ruiz S" first="S." last="Martin-Ruiz">S. Martin-Ruiz</name>
</country>
<country name="Grèce">
<region name="Attique (région)">
<name sortKey="Niarchos, P G" sort="Niarchos, P G" uniqKey="Niarchos P" first="P. G." last="Niarchos">P. G. Niarchos</name>
</region>
<name sortKey="Gazeas, K D" sort="Gazeas, K D" uniqKey="Gazeas K" first="K. D." last="Gazeas">K. D. Gazeas</name>
<name sortKey="Manimanis, V N" sort="Manimanis, V N" uniqKey="Manimanis V" first="V. N." last="Manimanis">V. N. Manimanis</name>
</country>
<country name="Belgique">
<region name="Vienne (Autriche)">
<name sortKey="Van Cauteren, P" sort="Van Cauteren, P" uniqKey="Van Cauteren P" first="P." last="Van Cauteren">P. Van Cauteren</name>
</region>
<name sortKey="Lampens, P" sort="Lampens, P" uniqKey="Lampens P" first="P." last="Lampens">P. Lampens</name>
<name sortKey="Wils, P" sort="Wils, P" uniqKey="Wils P" first="P." last="Wils">P. Wils</name>
</country>
<country name="France">
<noRegion>
<name sortKey="Van Cauteren, P" sort="Van Cauteren, P" uniqKey="Van Cauteren P" first="P." last="Van Cauteren">P. Van Cauteren</name>
</noRegion>
<name sortKey="Martignoni, M" sort="Martignoni, M" uniqKey="Martignoni M" first="M." last="Martignoni">M. Martignoni</name>
</country>
<country name="Chili">
<noRegion>
<name sortKey="Amado, P J" sort="Amado, P J" uniqKey="Amado P" first="P. J." last="Amado">P. J. Amado</name>
</noRegion>
</country>
<country name="Australie">
<noRegion>
<name sortKey="Butterworth, N D" sort="Butterworth, N D" uniqKey="Butterworth N" first="N. D." last="Butterworth">N. D. Butterworth</name>
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</country>
<country name="Pologne">
<noRegion>
<name sortKey="Moskalik, P" sort="Moskalik, P" uniqKey="Moskalik P" first="P." last="Moskalik">P. Moskalik</name>
</noRegion>
</country>
<country name="États-Unis">
<noRegion>
<name sortKey="Robertson, C W" sort="Robertson, C W" uniqKey="Robertson C" first="C. W." last="Robertson">C. W. Robertson</name>
</noRegion>
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</affiliations>
</record>

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