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Normal modes and discovery of high‐order cross‐frequencies in the DBV white dwarf GD 358

Identifieur interne : 00BF64 ( Main/Exploration ); précédent : 00BF63; suivant : 00BF65

Normal modes and discovery of high‐order cross‐frequencies in the DBV white dwarf GD 358

Auteurs : F. Vuille [Afrique du Sud, Suisse] ; D. O Onoghue [Afrique du Sud] ; D. A. H. Buckley [Afrique du Sud] ; C. Massacand [Norvège, Suisse] ; J. E. Solheim [Norvège] ; S. Bard [Norvège] ; G. Vauclair [France] ; O. Giovannini [Brésil, Suisse] ; S. O. Kepler [Brésil] ; A. Kanaan [Brésil] ; J. L. Provencal [États-Unis] ; M. A. Wood [États-Unis] ; J. C. Clemens [États-Unis] ; S. J. Kleinman [États-Unis, Suisse] ; M. S. O Rien [États-Unis] ; R. E. Nather [États-Unis] ; D. E. Winget [États-Unis] ; A. Nitta [États-Unis] ; E. W. Klumpe [États-Unis] ; M. H. Montgomery [États-Unis, Autriche] ; T. K. Watson [États-Unis] ; P. A. Bradley [États-Unis] ; D. J. Sullivan [Nouvelle-Zélande] ; K. Wu [Australie] ; T. M. K. Marar [Inde] ; S. Seetha [Inde] ; B. N. Ashoka [Inde] ; H. S. Mahra [Inde] ; B. C. Bhat [Inde] ; V. C. Babu [Inde] ; E. M. Leibowitz [Israël] ; S. Hemar [Israël] ; P. Ibbetson [Israël] ; E. Mashals [Israël] ; E. Meištas [Lituanie, Suisse] ; P. Moskalik [Pologne] ; S. Zoła [Pologne] ; J. Krzesi Ski [Pologne] ; G. Pajdosz [Pologne]

Source :

RBID : ISTEX:FC5B3F7923FD3368968E64D8A94F2AD30349B453

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English descriptors

Abstract

We present a detailed mode identification performed on the 1994 Whole Earth Telescope (WET) run on GD 358. The results are compared with that obtained for the same star from the 1990 WET data. The two temporal spectra show very few qualitative differences, although amplitude changes are seen in most modes, including the disappearance of the mode identified as k=14 in the 1990 data. The excellent coverage and signal‐to‐noise ratio obtained during the 1994 run lead to the secure identification of combination frequencies up to fourth order, i.e. peaks that are sums or differences of up to four parent frequencies, including a virtually complete set of second‐order frequencies, as expected from harmonic distortion. We show how the third‐order frequencies are expected to affect the triplet structure of the normal modes by back‐interacting with them. Finally, a search for ℓ=2 modes was unsuccessful, not verifying the suspicion that such modes had been uncovered in the 1990 data set.

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DOI: 10.1046/j.1365-8711.2000.03369.x


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<author>
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<author>
<name sortKey="Wu, K" sort="Wu, K" uniqKey="Wu K" first="K." last="Wu">K. Wu</name>
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<author>
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</author>
<author>
<name sortKey="Seetha, S" sort="Seetha, S" uniqKey="Seetha S" first="S." last="Seetha">S. Seetha</name>
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</author>
<author>
<name sortKey="Ashoka, B N" sort="Ashoka, B N" uniqKey="Ashoka B" first="B. N." last="Ashoka">B. N. Ashoka</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Inde</country>
<wicri:regionArea>Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017</wicri:regionArea>
<wicri:noRegion>Bangalore 560 017</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Mahra, H S" sort="Mahra, H S" uniqKey="Mahra H" first="H. S." last="Mahra">H. S. Mahra</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Inde</country>
<wicri:regionArea>Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017</wicri:regionArea>
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</author>
<author>
<name sortKey="Bhat, B C" sort="Bhat, B C" uniqKey="Bhat B" first="B. C." last="Bhat">B. C. Bhat</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Inde</country>
<wicri:regionArea>Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017</wicri:regionArea>
<wicri:noRegion>Bangalore 560 017</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Babu, V C" sort="Babu, V C" uniqKey="Babu V" first="V. C." last="Babu">V. C. Babu</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Inde</country>
<wicri:regionArea>Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017</wicri:regionArea>
<wicri:noRegion>Bangalore 560 017</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Leibowitz, E M" sort="Leibowitz, E M" uniqKey="Leibowitz E" first="E. M." last="Leibowitz">E. M. Leibowitz</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Israël</country>
<wicri:regionArea>University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978</wicri:regionArea>
<wicri:noRegion>Tel Aviv 69978</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Hemar, S" sort="Hemar, S" uniqKey="Hemar S" first="S." last="Hemar">S. Hemar</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Israël</country>
<wicri:regionArea>University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978</wicri:regionArea>
<wicri:noRegion>Tel Aviv 69978</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Ibbetson, P" sort="Ibbetson, P" uniqKey="Ibbetson P" first="P." last="Ibbetson">P. Ibbetson</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Israël</country>
<wicri:regionArea>University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978</wicri:regionArea>
<wicri:noRegion>Tel Aviv 69978</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Mashals, E" sort="Mashals, E" uniqKey="Mashals E" first="E." last="Mashals">E. Mashals</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Israël</country>
<wicri:regionArea>University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978</wicri:regionArea>
<wicri:noRegion>Tel Aviv 69978</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Meistas, E" sort="Meistas, E" uniqKey="Meistas E" first="E." last="Meištas">E. Meištas</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Lituanie</country>
<wicri:regionArea>Institute of Theoretical Physics and Astronomy, Goštauto 12, Vilnius 2600</wicri:regionArea>
<wicri:noRegion>Vilnius 2600</wicri:noRegion>
</affiliation>
<affiliation wicri:level="1">
<country wicri:rule="url">Suisse</country>
</affiliation>
</author>
<author>
<name sortKey="Moskalik, P" sort="Moskalik, P" uniqKey="Moskalik P" first="P." last="Moskalik">P. Moskalik</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Pologne</country>
<wicri:regionArea>Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00‐716 Warsaw</wicri:regionArea>
<wicri:noRegion>00‐716 Warsaw</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Zola, S" sort="Zola, S" uniqKey="Zola S" first="S." last="Zoła">S. Zoła</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Pologne</country>
<wicri:regionArea>Astronomical Observatory, Jagiellonian University, ul. Orla 171, 30‐244 Cracow</wicri:regionArea>
<wicri:noRegion>30‐244 Cracow</wicri:noRegion>
</affiliation>
<affiliation wicri:level="1">
<country xml:lang="fr">Pologne</country>
<wicri:regionArea>Mt Suhora Observatory, Cracow Pedagogical University, ul. Podchorazych 2, 30‐084 Cracow</wicri:regionArea>
<wicri:noRegion>30‐084 Cracow</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Krzesi Ski, J" sort="Krzesi Ski, J" uniqKey="Krzesi Ski J" first="J." last="Krzesi Ski">J. Krzesi Ski</name>
<affiliation wicri:level="1">
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<wicri:regionArea>Mt Suhora Observatory, Cracow Pedagogical University, ul. Podchorazych 2, 30‐084 Cracow</wicri:regionArea>
<wicri:noRegion>30‐084 Cracow</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Pajdosz, G" sort="Pajdosz, G" uniqKey="Pajdosz G" first="G." last="Pajdosz">G. Pajdosz</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Pologne</country>
<wicri:regionArea>Mt Suhora Observatory, Cracow Pedagogical University, ul. Podchorazych 2, 30‐084 Cracow</wicri:regionArea>
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<monogr></monogr>
<series>
<title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title>
<title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title>
<idno type="ISSN">0035-8711</idno>
<idno type="eISSN">1365-2966</idno>
<imprint>
<biblScope unit="vol">314</biblScope>
<biblScope unit="issue">4</biblScope>
<biblScope unit="page" from="689">689</biblScope>
<biblScope unit="page" to="701">701</biblScope>
<biblScope unit="page-count">13</biblScope>
<publisher>Blackwell Science Ltd</publisher>
<pubPlace>Oxford, UK</pubPlace>
<date type="published" when="2000-06">2000-06</date>
</imprint>
<idno type="ISSN">0035-8711</idno>
</series>
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<idno type="ISSN">0035-8711</idno>
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<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Amplitude</term>
<term>Amplitude modulation</term>
<term>Amplitude spectrum</term>
<term>Arrowhead</term>
<term>Azimuthal order</term>
<term>Bradley winget</term>
<term>Brassard</term>
<term>Cent coverage</term>
<term>Central peak</term>
<term>Combination frequencies</term>
<term>Combination modes</term>
<term>Combination multiplets</term>
<term>Difference frequencies</term>
<term>Different modes</term>
<term>Excellent coverage</term>
<term>First column</term>
<term>Frequency</term>
<term>Frequency splitting</term>
<term>Ftpt</term>
<term>Goupil serre</term>
<term>Guest observer</term>
<term>Harmonic</term>
<term>Harmonic distortion</term>
<term>Highest peak</term>
<term>Inverse variance</term>
<term>Inverse variance method</term>
<term>Larger peaks</term>
<term>Last column</term>
<term>Light curve</term>
<term>Mauna</term>
<term>Mcdonald</term>
<term>Mnras</term>
<term>Mode</term>
<term>Mode identification</term>
<term>Multiplet</term>
<term>Multiplet structures</term>
<term>Multiplets</term>
<term>Nather</term>
<term>Noise level</term>
<term>Normal modes</term>
<term>Numerous combination frequencies</term>
<term>Parent multiplets</term>
<term>Peak</term>
<term>Period spacing</term>
<term>Period spectrum</term>
<term>Possible identifications</term>
<term>Possible identifications identification</term>
<term>Possible ones</term>
<term>Probable origin</term>
<term>Prograde</term>
<term>Prograde component</term>
<term>Prograde mode</term>
<term>Progress report</term>
<term>Radial order</term>
<term>Resonant mode</term>
<term>Right panel</term>
<term>Saao</term>
<term>Saao itajuba mauna</term>
<term>Search procedure</term>
<term>Second order</term>
<term>Significant power</term>
<term>Simple triplet structure</term>
<term>Small peaks</term>
<term>Spacing</term>
<term>Spectral window</term>
<term>Spring nainital</term>
<term>Spring saao</term>
<term>Straightforward exercise</term>
<term>Suhora</term>
<term>Suhora mcdonald mauna</term>
<term>Synthetic light curve</term>
<term>Telescope mauna</term>
<term>Temporal spectrum</term>
<term>Theoretical astrophysics</term>
<term>Theoretical model</term>
<term>Third column</term>
<term>Third order</term>
<term>Triplet</term>
<term>Variance</term>
<term>Vuille</term>
<term>Vuille brassard</term>
<term>Whole earth telescope</term>
<term>Winget</term>
<term>Winget fontaine</term>
<term>stars: individual: GD 358</term>
<term>stars: variables: other</term>
<term>white dwarfs</term>
</keywords>
<keywords scheme="Teeft" xml:lang="en">
<term>Amplitude</term>
<term>Amplitude modulation</term>
<term>Amplitude spectrum</term>
<term>Arrowhead</term>
<term>Azimuthal order</term>
<term>Bradley winget</term>
<term>Brassard</term>
<term>Cent coverage</term>
<term>Central peak</term>
<term>Combination frequencies</term>
<term>Combination modes</term>
<term>Combination multiplets</term>
<term>Difference frequencies</term>
<term>Different modes</term>
<term>Excellent coverage</term>
<term>First column</term>
<term>Frequency</term>
<term>Frequency splitting</term>
<term>Ftpt</term>
<term>Goupil serre</term>
<term>Guest observer</term>
<term>Harmonic</term>
<term>Harmonic distortion</term>
<term>Highest peak</term>
<term>Inverse variance</term>
<term>Inverse variance method</term>
<term>Larger peaks</term>
<term>Last column</term>
<term>Light curve</term>
<term>Mauna</term>
<term>Mcdonald</term>
<term>Mnras</term>
<term>Mode</term>
<term>Mode identification</term>
<term>Multiplet</term>
<term>Multiplet structures</term>
<term>Multiplets</term>
<term>Nather</term>
<term>Noise level</term>
<term>Normal modes</term>
<term>Numerous combination frequencies</term>
<term>Parent multiplets</term>
<term>Peak</term>
<term>Period spacing</term>
<term>Period spectrum</term>
<term>Possible identifications</term>
<term>Possible identifications identification</term>
<term>Possible ones</term>
<term>Probable origin</term>
<term>Prograde</term>
<term>Prograde component</term>
<term>Prograde mode</term>
<term>Progress report</term>
<term>Radial order</term>
<term>Resonant mode</term>
<term>Right panel</term>
<term>Saao</term>
<term>Saao itajuba mauna</term>
<term>Search procedure</term>
<term>Second order</term>
<term>Significant power</term>
<term>Simple triplet structure</term>
<term>Small peaks</term>
<term>Spacing</term>
<term>Spectral window</term>
<term>Spring nainital</term>
<term>Spring saao</term>
<term>Straightforward exercise</term>
<term>Suhora</term>
<term>Suhora mcdonald mauna</term>
<term>Synthetic light curve</term>
<term>Telescope mauna</term>
<term>Temporal spectrum</term>
<term>Theoretical astrophysics</term>
<term>Theoretical model</term>
<term>Third column</term>
<term>Third order</term>
<term>Triplet</term>
<term>Variance</term>
<term>Vuille</term>
<term>Vuille brassard</term>
<term>Whole earth telescope</term>
<term>Winget</term>
<term>Winget fontaine</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr">
<term>Niveau sonore</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">We present a detailed mode identification performed on the 1994 Whole Earth Telescope (WET) run on GD 358. The results are compared with that obtained for the same star from the 1990 WET data. The two temporal spectra show very few qualitative differences, although amplitude changes are seen in most modes, including the disappearance of the mode identified as k=14 in the 1990 data. The excellent coverage and signal‐to‐noise ratio obtained during the 1994 run lead to the secure identification of combination frequencies up to fourth order, i.e. peaks that are sums or differences of up to four parent frequencies, including a virtually complete set of second‐order frequencies, as expected from harmonic distortion. We show how the third‐order frequencies are expected to affect the triplet structure of the normal modes by back‐interacting with them. Finally, a search for ℓ=2 modes was unsuccessful, not verifying the suspicion that such modes had been uncovered in the 1990 data set.</div>
</front>
</TEI>
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<li>Norvège</li>
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<li>Suisse</li>
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<li>Rio Grande do Sul</li>
<li>Santa Catarina</li>
<li>Texas</li>
</region>
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<li>Ames (Iowa)</li>
<li>Austin (Texas)</li>
<li>Porto Alegre</li>
<li>Sydney</li>
<li>Toulouse</li>
</settlement>
<orgName>
<li>Université d'État de l'Iowa</li>
<li>Université de Sydney</li>
<li>Université du Texas à Austin</li>
<li>Université fédérale du Rio Grande do Sul</li>
</orgName>
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<name sortKey="Meistas, E" sort="Meistas, E" uniqKey="Meistas E" first="E." last="Meištas">E. Meištas</name>
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<name sortKey="Solheim, J E" sort="Solheim, J E" uniqKey="Solheim J" first="J. E." last="Solheim">J. E. Solheim</name>
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<country name="France">
<region name="Occitanie (région administrative)">
<name sortKey="Vauclair, G" sort="Vauclair, G" uniqKey="Vauclair G" first="G." last="Vauclair">G. Vauclair</name>
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</country>
<country name="Brésil">
<region name="Rio Grande do Sul">
<name sortKey="Giovannini, O" sort="Giovannini, O" uniqKey="Giovannini O" first="O." last="Giovannini">O. Giovannini</name>
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<name sortKey="Kanaan, A" sort="Kanaan, A" uniqKey="Kanaan A" first="A." last="Kanaan">A. Kanaan</name>
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<name sortKey="Kleinman, S J" sort="Kleinman, S J" uniqKey="Kleinman S" first="S. J." last="Kleinman">S. J. Kleinman</name>
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<name sortKey="Ibbetson, P" sort="Ibbetson, P" uniqKey="Ibbetson P" first="P." last="Ibbetson">P. Ibbetson</name>
<name sortKey="Mashals, E" sort="Mashals, E" uniqKey="Mashals E" first="E." last="Mashals">E. Mashals</name>
</country>
<country name="Lituanie">
<noRegion>
<name sortKey="Meistas, E" sort="Meistas, E" uniqKey="Meistas E" first="E." last="Meištas">E. Meištas</name>
</noRegion>
</country>
<country name="Pologne">
<noRegion>
<name sortKey="Moskalik, P" sort="Moskalik, P" uniqKey="Moskalik P" first="P." last="Moskalik">P. Moskalik</name>
</noRegion>
<name sortKey="Krzesi Ski, J" sort="Krzesi Ski, J" uniqKey="Krzesi Ski J" first="J." last="Krzesi Ski">J. Krzesi Ski</name>
<name sortKey="Pajdosz, G" sort="Pajdosz, G" uniqKey="Pajdosz G" first="G." last="Pajdosz">G. Pajdosz</name>
<name sortKey="Zola, S" sort="Zola, S" uniqKey="Zola S" first="S." last="Zoła">S. Zoła</name>
<name sortKey="Zola, S" sort="Zola, S" uniqKey="Zola S" first="S." last="Zoła">S. Zoła</name>
</country>
</tree>
</affiliations>
</record>

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