The pulsations of PG 1351+489

M. Redaelli,S. O. Kepler,Jörge E S Costa,Don E. Winget,Gerald Handler,Bárbara Garcia Castanheira,Antonio Kanaan,Luciano Fraga,P. Henrique,Odilon Giovannini,Judi L. Provençal,Harry L. Shipman,James Dalessio,Susan E. Thompson,Fergal R. Mullally,M. M. Brewer,D. Childers,Mary E. Oksala,Rachel A. Rosen,Matt A. Wood,Mike D. Reed,B. Walter,W. Strickland,Dean W. Chandler,Todd K. Watson,R. Edward Nather,Michael H. Montgomery,Agnès Bischoff-Kim,Carl J. Hansen,Atsuko Nitta,Scot J. Kleinman,Charles F. Claver,Timothy M. Brown,Denis J. Sullivan,Seunglee Kim,Wenping Chen,Mingchung Yang,ChiaYou Shih,Xiaobin Zhang,Xiaojun Jiang,Jianning Fu,S. Seetha, B. N. Ashoka,T. M K Marar,K. S. Baliyan,Hari Om Vats,Andrei V. Chernyshev,P. A. Ibbetson,Elia M. Leibowitz,Shirley Hemar,Aleksandre V. Sergeev,Maksim V. Andreev,Rimvydas Janulis,E. G. Meištas,Paweł A. Moskalik,G. Pajdosz,Andrzej S. Baran,Maciej Winiarski,Stanislaw Zoła,Waldemar Ogłoza,Michał Siwak,Zs Bognár,Jan Erik Solheim,Ramotholo R. Sefako,David A H Buckley,Darragh E. O'Donoghue,Thorsten Nagel,Roberto Silvotti,Ivan Bruni, J. R. Fremy,Gérard P. Vauclair,M. Chevreton,Noël Dolez,Burkhard R K Pfeiffer,Martin A. Barstow,Orlagh L. Creevey,Steven D. Kawaler,J. Christopher Clemens

Monthly Notices of the Royal Astronomical Society（2011）

引用 14|浏览94

暂无评分

摘要

PG 1351+489 is one of the 20 DBVs – pulsating helium-atmosphere white dwarf stars – known and has the simplest power spectrum for this class of star, making it a good candidate to study cooling rates. We report accurate period determinations for the main peak at 489.334 48 s and two other normal modes using data from the Whole Earth Telescope (WET) observations of 1995 and 2009. In 2009, we detect...

查看译文

关键词

stars: evolution,stars: individual: PG 1351+489,stars: oscillations,white dwarfs

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要