Open Astronomy (Mar 2003)
Wet Observations of GD 358 in 2000
- Kepler S. O.,
- Nather E.R.,
- Winget D.E.,
- Nitta A.,
- Kleinman S.J.,
- Metcalfe T.,
- Sekiguchi K.,
- Xiaojun J.,
- Sullivan D.,
- Sullivan T.,
- Janulis R.,
- Meištas E.G.,
- Kalytis R.,
- Krzesiński J.,
- Ogłoza W.,
- Zola S.,
- O’Donoghue D.,
- Romero-Colmenero E.,
- Martinez P.,
- Dreizler S.,
- Deetjen J.,
- Nagel T.,
- Schuh S.L.,
- Vauclair G.,
- Fu J.N.,
- Chevreton M.,
- Solheim J.-E.,
- Kanaan A.,
- Costa J.E.,
- Costa A.F. Murillo,
- Wood M.A.,
- Silvestri N.,
- Ahrens T.J.,
- Jones A. Kyle,
- Collins A.E.,
- Boyer M.,
- Shaw J.S.,
- Mukadam A.S.,
- Klumpe E.W.,
- Larrison J.,
- Kawaler S.D.,
- Riddle R.L.,
- Ulla A.,
- Bradley P.
Affiliations
- Kepler S. O.
- Instituto de Física da UFRGS, Porto Alegre, RS, Brazil
- Nather E.R.
- Department of Astronomy and McDonald Observatory, University of Texas, Austin, TX 78712, United States of America
- Winget D.E.
- Department of Astronomy and McDonald Observatory, University of Texas, Austin, TX 78712, United States of America
- Nitta A.
- Sloan Digital Sky Survey, Apache Pt. Observatory, P.O. Box 59, Sunspot, NM 88349, United States of America
- Kleinman S.J.
- Sloan Digital Sky Survey, Apache Pt. Observatory, P.O. Box 59, Sunspot, NM 88349, United States of America
- Metcalfe T.
- Department of Astronomy and McDonald Observatory, University of Texas, Austin, TX 78712, U.S.A. United States of America
- Sekiguchi K.
- Subaru National Astronomical Observatory of Japan, Hawaii, United States of America
- Xiaojun J.
- Beijing Astronomical Observatory, Academy of Sciences, Beijing 100080, China
- Sullivan D.
- University of Victoria, Wellington, New Zealand
- Sullivan T.
- University of Victoria, Wellington, New Zealand
- Janulis R.
- Institute of Theoretical Physics and Astronomy, Goˇstauto 12, Vilnius 2600, Lithuania
- Meištas E.G.
- Institute of Theoretical Physics and Astronomy, Goˇstauto 12, Vilnius 2600, Lithuania
- Kalytis R.
- Vilnius University Astronomical Observatory, Čiurlionio 29, Vilnius 2009, Lithuania
- Krzesiński J.
- Mt. Suhora Observatory, Cracow Pedagogical University, Ul. Podchorazych 2, 30-084 Cracow, Poland
- Ogłoza W.
- Mt. Suhora Observatory, Cracow Pedagogical University, Ul. Podchorazych 2, 30-084 Cracow, Poland
- Zola S.
- Jagiellonian University, ul. Orla 171, 30-244 Cracow, Poland
- O’Donoghue D.
- South African Astronomical Observatory, Cape Town, South Africa
- Romero-Colmenero E.
- South African Astronomical Observatory, Cape Town, South Africa
- Martinez P.
- South African Astronomical Observatory, Cape Town, South Africa
- Dreizler S.
- Institut für Astronomie und Astrophysik, Universität, Sand 1, D-72076, Tübingen, Germany
- Deetjen J.
- Institut für Astronomie und Astrophysik, Universität, Sand 1, D-72076, Tübingen, Germany
- Nagel T.
- Institut für Astronomie und Astrophysik, Universität, Sand 1, D-72076, Tübingen, Germany
- Schuh S.L.
- Institut für Astronomie und Astrophysik, Universität, Sand 1, D-72076, Tübingen, Germany
- Vauclair G.
- Université Paul Sabatier, Observatoire Midi-Pyrénées, CNRS/UMR5572, 14 av. E. Belin, 31400 Toulouse, France
- Fu J.N.
- Université Paul Sabatier, Observatoire Midi-Pyrénées, CNRS/UMR5572, 14 av. E. Belin, 31400 Toulouse, France
- Chevreton M.
- Observatoire de Paris-Meudon, DAEC, 92195 Meudon, France
- Solheim J.-E.
- Institutt for Fysikk, Universitet i Tromsø 9037 Tromsø, Norway
- Kanaan A.
- Departamento de Física, Universidade Federal de Santa Catarina, CP 476, CEP 88040-900, Florianópolis, Brazil
- Costa J.E.
- Instituto de Física da UFRGS, Porto Alegre, RS, Brazil
- Costa A.F. Murillo
- Instituto de Física da UFRGS, Porto Alegre, RS, Brazil
- Wood M.A.
- Dept. of Physics and Space Sciences & The SARA Observatory, Florida Institute of Technology, Melbourne, FL 32901, United States of America
- Silvestri N.
- Dept. of Physics and Space Sciences & The SARA Observatory, Florida Institute of Technology, Melbourne, FL 32901, United States of America
- Ahrens T.J.
- Dept. of Physics and Space Sciences & The SARA Observatory, Florida Institute of Technology, Melbourne, FL 32901, United States of America
- Jones A. Kyle
- University of Florida, 202 Nuclear Sciences Center Gainesville, FL 32611-8300, United States of America
- Collins A.E.
- Johnson Space Center, 2101 NASA Road 1, Mail Code GT2, Houston, TX 77058, United States of America
- Boyer M.
- University of Minnesota, Department of Physics & Astronomy, 116 Church St. S.E., Minneapolis, MN 55455, Unites States of America
- Shaw J.S.
- University of Georgia at Athens, Department of Physics and Astronomy, Athens, GA 30602-2451, United States of America
- Mukadam A.S.
- Department of Astronomy and McDonald Observatory, University of Texas, Austin, TX 78712, United States of America
- Klumpe E.W.
- Middle Tennessee State University, Department of Physics and Astronomy Murfreesboro, TN 37132, United States of America
- Larrison J.
- Middle Tennessee State University, Department of Physics and Astronomy Murfreesboro, TN 37132, United States of America
- Kawaler S.D.
- Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, United States of America
- Riddle R.L.
- Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, United States of America
- Ulla A.
- Universidade de Vigo, Depto. de Fisica Aplicada, Facultade de Ciencias, Campus Marcosende-Lagoas, 36200 Vigo (Pontevedra), Spain
- Bradley P.
- Los Alamos National Laboratory, X-2, MS T-085 Los Alamos, NM 87545, United States of America
- DOI
- https://doi.org/10.1515/astro-2017-0033
- Journal volume & issue
-
Vol. 12,
no. 1
pp. 45 – 53
Abstract
We report on the 323 hours of nearly uninterrupted time series photometric observations of the DBV star GD 358 acquired with the Whole Earth Telescope (WET) during May 23 to June 8, 2000. We acquired more than 232 000 independent measurements and detected the non-radial g-modes consistent with degree ℓ = 1 and radial order 8 to 20 and their linear combinations up to 6th order. We also detect, for the first time, a high amplitude ℓ = 2 mode, with a period of 796 s. In the 2000 WET data, the largest amplitude modes are similar to those detected with the WET observations of 1990 and 1994, but the highest combination order previously detected was 4th order.
Keywords
