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20 April 2024
 
  » arxiv » astro-ph/0511827

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Resolving the pulsations of the subdwarf B star KPD 2109+4401
A.-Y. Zhou ; M.D. Reed ; S. Harms ; D.M. Terndrup ; D. An ; S. Zola ; K. D. Gazeas ; P. G. Niarchos ; W. Ogloza ; A. Baran ; G. W. Wolf ;
Date 30 Nov 2005
Journal Mon.Not.Roy.Astron.Soc. 367 (2006) 179-185
AbstractWe present the results of extensive time series photometry of the pulsating subdwarf B star KPD 2109+4401. Our data set consists of 29 data runs with a total length of 182.6 hours over 31 days, collected at five observatories in 2004. These data are comprised of high signal-to-noise observations acquired with larger telescopes and wider time coverage observations obtained with smaller telescopes. They are sufficient to resolve the pulsation structure to 0.4 $mu$Hz and are the most extensive data set for this star to date. With these data, we identify eight pulsation frequencies extending from 4701 to 5481 $mu$Hz, corresponding to periods of 182 to 213 s. The pulsation frequencies and their amplitudes are examined over several time-scales with some frequencies showing amplitude variability.
Source arXiv, astro-ph/0511827
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