Normal modes and discovery of high-order cross-frequencies in the DBV white dwarf GD 358
Corresponding Author
F. Vuille
Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa
★ Present address: Eterpy 49, 1020 Renens, Switzerland.† E-mail: [email protected]‡ Guest observer at Assey-Turgen Observatory, Kazakhstan.§ Visiting astronomer at the Laboratorio Nacional de Astrofisica/CNPq, Brazil.¶ Guest observer at Siding Spring Observatory, Australia.Search for more papers by this authorD. O’Donoghue
South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa
Search for more papers by this authorD. A. H. Buckley
South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa
Search for more papers by this authorCorresponding Author
C.-M. Massacand
MR, Nordlysobservatoriet, Universitetet i Tromso, N-9037 Tromso, Norway
★ Present address: Eterpy 49, 1020 Renens, Switzerland.† E-mail: [email protected]‡ Guest observer at Assey-Turgen Observatory, Kazakhstan.§ Visiting astronomer at the Laboratorio Nacional de Astrofisica/CNPq, Brazil.¶ Guest observer at Siding Spring Observatory, Australia.Search for more papers by this authorJ. E. Solheim
MR, Nordlysobservatoriet, Universitetet i Tromso, N-9037 Tromso, Norway
Search for more papers by this authorS. Bard
University of Oslo, Institute of Theoretical Astrophysics, PO Box 1029 – Blindern, N-0315 Oslo, Norway
Search for more papers by this authorG. Vauclair
Observatoire Midi-Pyrenees, 14 Avenue E. Belin, 31400 Toulouse, France
Search for more papers by this authorCorresponding Author
O. Giovannini
Instituto de Fisica, Universidade Federal do Rio Grande do Sul, 91500-970 Porto Alegre RS, Brazil
★ Present address: Eterpy 49, 1020 Renens, Switzerland.† E-mail: [email protected]‡ Guest observer at Assey-Turgen Observatory, Kazakhstan.§ Visiting astronomer at the Laboratorio Nacional de Astrofisica/CNPq, Brazil.¶ Guest observer at Siding Spring Observatory, Australia.Search for more papers by this authorS. O. Kepler
Instituto de Fisica, Universidade Federal do Rio Grande do Sul, 91500-970 Porto Alegre RS, Brazil
Search for more papers by this authorA. Kanaan
Dep. de Fisica – UFSC, Campus Universitario – Trindade, CEP 88040-900 – Florianopolis SC, Brazil
Search for more papers by this authorJ. L. Provencal
Sharp Laboratory, Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, USA
Search for more papers by this authorM. A. Wood
Department of Physics and Space Sciences, Florida Institute of Technology, 150 W. University Blvd, Melbourne, FL 32901-6975, USA
Search for more papers by this authorJ. C. Clemens
Campus Box 3255, 264 Phillips Hall, Chapel Hill, NC 27599, USA
Search for more papers by this authorCorresponding Author
S. J. Kleinman
Iowa State University, Department of Physics and Astronomy, Ames, IA 50011, USA
★ Present address: Eterpy 49, 1020 Renens, Switzerland.† E-mail: [email protected]‡ Guest observer at Assey-Turgen Observatory, Kazakhstan.§ Visiting astronomer at the Laboratorio Nacional de Astrofisica/CNPq, Brazil.¶ Guest observer at Siding Spring Observatory, Australia.Search for more papers by this authorM. S. O’Brien
Department of Physics, Grinnell College, PO Box 805, Grinnell, IA 50112-0806, USA
Search for more papers by this authorR. E. Nather
Astronomy Department, University of Texas at Austin, Austin, TX 78712, USA
Search for more papers by this authorD. E. Winget
Astronomy Department, University of Texas at Austin, Austin, TX 78712, USA
Search for more papers by this authorA. Nitta
Astronomy Department, University of Texas at Austin, Austin, TX 78712, USA
Search for more papers by this authorE. W. Klumpe
Astronomy Department, University of Texas at Austin, Austin, TX 78712, USA
Search for more papers by this authorM. H. Montgomery
Astronomy Department, University of Texas at Austin, Austin, TX 78712, USA
Institute for Astronomy, Türkenschanzstraße 17, A-1180 Vienna, Austria
Search for more papers by this authorT. K. Watson
Information Technology Services, Southwestern University, Georgetown, TX 78626, USA
Search for more papers by this authorP. A. Bradley
XTA, MS B220, Los Alamos National Laboratory, Los Alamos, NM 874545, USA
Search for more papers by this authorD. J. Sullivan
Department of Physics, Victoria University of Wellington, PO Box 600, Wellington, New Zealand
Search for more papers by this authorK. Wu
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, Australia
Search for more papers by this authorT. M. K. Marar
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorS. Seetha
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorB. N. Ashoka
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorH. S. Mahra
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorB. C. Bhat
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorV. C. Babu
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorE. M. Leibowitz
University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978, Israel
Search for more papers by this authorS. Hemar
University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978, Israel
Search for more papers by this authorP. Ibbetson
University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978, Israel
Search for more papers by this authorE. Mashals
University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978, Israel
Search for more papers by this authorCorresponding Author
E. Meištas
Institute of Theoretical Physics and Astronomy, Goštauto 12, Vilnius 2600, Lithuania
★ Present address: Eterpy 49, 1020 Renens, Switzerland.† E-mail: [email protected]‡ Guest observer at Assey-Turgen Observatory, Kazakhstan.§ Visiting astronomer at the Laboratorio Nacional de Astrofisica/CNPq, Brazil.¶ Guest observer at Siding Spring Observatory, Australia.Search for more papers by this authorP. Moskalik
Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland
Search for more papers by this authorS. Zoła
Astronomical Observatory, Jagiellonian University, ul. Orla 171, 30-244 Cracow, Poland
Mt Suhora Observatory, Cracow Pedagogical University, ul. Podchorazych 2, 30-084 Cracow, Poland
Search for more papers by this authorJ. Krzesiński
Mt Suhora Observatory, Cracow Pedagogical University, ul. Podchorazych 2, 30-084 Cracow, Poland
Search for more papers by this authorG. Pajdosz
Mt Suhora Observatory, Cracow Pedagogical University, ul. Podchorazych 2, 30-084 Cracow, Poland
Search for more papers by this authorCorresponding Author
F. Vuille
Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa
★ Present address: Eterpy 49, 1020 Renens, Switzerland.† E-mail: [email protected]‡ Guest observer at Assey-Turgen Observatory, Kazakhstan.§ Visiting astronomer at the Laboratorio Nacional de Astrofisica/CNPq, Brazil.¶ Guest observer at Siding Spring Observatory, Australia.Search for more papers by this authorD. O’Donoghue
South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa
Search for more papers by this authorD. A. H. Buckley
South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa
Search for more papers by this authorCorresponding Author
C.-M. Massacand
MR, Nordlysobservatoriet, Universitetet i Tromso, N-9037 Tromso, Norway
★ Present address: Eterpy 49, 1020 Renens, Switzerland.† E-mail: [email protected]‡ Guest observer at Assey-Turgen Observatory, Kazakhstan.§ Visiting astronomer at the Laboratorio Nacional de Astrofisica/CNPq, Brazil.¶ Guest observer at Siding Spring Observatory, Australia.Search for more papers by this authorJ. E. Solheim
MR, Nordlysobservatoriet, Universitetet i Tromso, N-9037 Tromso, Norway
Search for more papers by this authorS. Bard
University of Oslo, Institute of Theoretical Astrophysics, PO Box 1029 – Blindern, N-0315 Oslo, Norway
Search for more papers by this authorG. Vauclair
Observatoire Midi-Pyrenees, 14 Avenue E. Belin, 31400 Toulouse, France
Search for more papers by this authorCorresponding Author
O. Giovannini
Instituto de Fisica, Universidade Federal do Rio Grande do Sul, 91500-970 Porto Alegre RS, Brazil
★ Present address: Eterpy 49, 1020 Renens, Switzerland.† E-mail: [email protected]‡ Guest observer at Assey-Turgen Observatory, Kazakhstan.§ Visiting astronomer at the Laboratorio Nacional de Astrofisica/CNPq, Brazil.¶ Guest observer at Siding Spring Observatory, Australia.Search for more papers by this authorS. O. Kepler
Instituto de Fisica, Universidade Federal do Rio Grande do Sul, 91500-970 Porto Alegre RS, Brazil
Search for more papers by this authorA. Kanaan
Dep. de Fisica – UFSC, Campus Universitario – Trindade, CEP 88040-900 – Florianopolis SC, Brazil
Search for more papers by this authorJ. L. Provencal
Sharp Laboratory, Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, USA
Search for more papers by this authorM. A. Wood
Department of Physics and Space Sciences, Florida Institute of Technology, 150 W. University Blvd, Melbourne, FL 32901-6975, USA
Search for more papers by this authorJ. C. Clemens
Campus Box 3255, 264 Phillips Hall, Chapel Hill, NC 27599, USA
Search for more papers by this authorCorresponding Author
S. J. Kleinman
Iowa State University, Department of Physics and Astronomy, Ames, IA 50011, USA
★ Present address: Eterpy 49, 1020 Renens, Switzerland.† E-mail: [email protected]‡ Guest observer at Assey-Turgen Observatory, Kazakhstan.§ Visiting astronomer at the Laboratorio Nacional de Astrofisica/CNPq, Brazil.¶ Guest observer at Siding Spring Observatory, Australia.Search for more papers by this authorM. S. O’Brien
Department of Physics, Grinnell College, PO Box 805, Grinnell, IA 50112-0806, USA
Search for more papers by this authorR. E. Nather
Astronomy Department, University of Texas at Austin, Austin, TX 78712, USA
Search for more papers by this authorD. E. Winget
Astronomy Department, University of Texas at Austin, Austin, TX 78712, USA
Search for more papers by this authorA. Nitta
Astronomy Department, University of Texas at Austin, Austin, TX 78712, USA
Search for more papers by this authorE. W. Klumpe
Astronomy Department, University of Texas at Austin, Austin, TX 78712, USA
Search for more papers by this authorM. H. Montgomery
Astronomy Department, University of Texas at Austin, Austin, TX 78712, USA
Institute for Astronomy, Türkenschanzstraße 17, A-1180 Vienna, Austria
Search for more papers by this authorT. K. Watson
Information Technology Services, Southwestern University, Georgetown, TX 78626, USA
Search for more papers by this authorP. A. Bradley
XTA, MS B220, Los Alamos National Laboratory, Los Alamos, NM 874545, USA
Search for more papers by this authorD. J. Sullivan
Department of Physics, Victoria University of Wellington, PO Box 600, Wellington, New Zealand
Search for more papers by this authorK. Wu
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, Australia
Search for more papers by this authorT. M. K. Marar
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorS. Seetha
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorB. N. Ashoka
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorH. S. Mahra
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorB. C. Bhat
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorV. C. Babu
Technical Physics Divison, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
Search for more papers by this authorE. M. Leibowitz
University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978, Israel
Search for more papers by this authorS. Hemar
University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978, Israel
Search for more papers by this authorP. Ibbetson
University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978, Israel
Search for more papers by this authorE. Mashals
University of Tel Aviv, Department of Physics and Astronomy, Ramat Aviv, Tel Aviv 69978, Israel
Search for more papers by this authorCorresponding Author
E. Meištas
Institute of Theoretical Physics and Astronomy, Goštauto 12, Vilnius 2600, Lithuania
★ Present address: Eterpy 49, 1020 Renens, Switzerland.† E-mail: [email protected]‡ Guest observer at Assey-Turgen Observatory, Kazakhstan.§ Visiting astronomer at the Laboratorio Nacional de Astrofisica/CNPq, Brazil.¶ Guest observer at Siding Spring Observatory, Australia.Search for more papers by this authorP. Moskalik
Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland
Search for more papers by this authorS. Zoła
Astronomical Observatory, Jagiellonian University, ul. Orla 171, 30-244 Cracow, Poland
Mt Suhora Observatory, Cracow Pedagogical University, ul. Podchorazych 2, 30-084 Cracow, Poland
Search for more papers by this authorJ. Krzesiński
Mt Suhora Observatory, Cracow Pedagogical University, ul. Podchorazych 2, 30-084 Cracow, Poland
Search for more papers by this authorG. Pajdosz
Mt Suhora Observatory, Cracow Pedagogical University, ul. Podchorazych 2, 30-084 Cracow, Poland
Search for more papers by this authorAbstract
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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