A survey for pulsating subdwarf B stars with the Nordic Optical Telescope

被引:57
|
作者
Ostensen, R. H. [1 ]
Oreiro, R. [1 ]
Solheim, J. -E. [2 ]
Heber, U. [3 ]
Silvotti, R. [4 ]
Gonzalez-Perez, J. M. [5 ]
Ulla, A. [6 ]
Perez Hernandez, F. [5 ,7 ]
Rodriguez-Lopez, C. [6 ,8 ]
Telting, J. H. [9 ]
机构
[1] Katholieke Univ Leuven, Inst Sterrenkunde, B-3001 Louvain, Belgium
[2] Univ Oslo, Inst Teoret Astrofysikk, N-0212 Blindern Oslo, Norway
[3] Univ Erlangen Nurnberg, Astron Inst, Dr Remeis Sternwarte, D-96049 Bamberg, Germany
[4] Osserv Astron Torino, INAF, I-10025 Pino Torinese, Italy
[5] Inst Astrofis Canarias, Tenerife 38200, Spain
[6] Univ Vigo, Dept Fis Aplicada, Vigo 36310, Spain
[7] Univ La Laguna, Dept Astrofis, Tenerife 38205, Spain
[8] Univ Toulouse, Lab Astrophys Toulouse Tarbes, F-31400 Toulouse, France
[9] Nord Opt Telescope, Santa Cruz De La Palma 38700, Spain
基金
欧洲研究理事会;
关键词
subdwarfs; surveys; stars: oscillations; EC; 14026; STARS; WHOLE EARTH TELESCOPE; FOLLOW-UP OBSERVATIONS; P-MODE PULSATIONS; SDB STAR; WHITE-DWARF; ATMOSPHERIC PARAMETERS; ASTEROSEISMIC ANALYSIS; MULTISITE CAMPAIGN; SPECTRAL-ANALYSIS;
D O I
10.1051/0004-6361/200913480
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Context. A search programme for pulsating subdwarf B stars was conducted with the Nordic Optical Telescope on La Palma over 59 nights between 1999 and 2009. Aims. The purpose of the programme was to significantly extend the number of rapidly pulsating sdB stars to better understand the properties of this new group of variable compact stars. Methods. Candidates were selected initially from the HS and HE surveys, but were supplemented with additional objects from other surveys. Short sequences of time-series photometry were made on the candidates to determine the presence of rapid pulsations. Results. In total twenty new pulsators were found in this survey, most of which have already been published and some extensively studied. We present four new short period pulsators, bringing the total of such pulsators up to 49. We also give limits on pulsation amplitudes for 285 objects with no obvious periodic variations, summarise the results of the survey, and provide improved physical parameters on the composite pulsators for which only preliminary estimates were published earlier.
引用
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页数:15
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