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Astrophysics and Space Science

, Volume 329, Issue 1–2, pp 211–216 | Cite as

Synthetic pulsational line profile variations

  • R. OreiroEmail author
  • J. H. Telting
  • R. H. Østensen
  • M. Briquet
  • C. Aerts
  • U. Heber
  • M. Vučković
Original Article
  • 56 Downloads

Abstract

We have produced simulated time series of high resolution spectroscopy for sdBs. We present the first results of testing classical mode identification techniques. Here, in particular, we analyse the behaviour of individual spectral lines and discuss the results and applicability of the moment method.

Keywords

Asteroseismology Hot subdwarfs 

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Copyright information

© Springer Science+Business Media B.V. 2010

Authors and Affiliations

  • R. Oreiro
    • 1
    Email author
  • J. H. Telting
    • 3
  • R. H. Østensen
    • 1
  • M. Briquet
    • 1
  • C. Aerts
    • 1
    • 2
  • U. Heber
    • 4
  • M. Vučković
    • 1
  1. 1.Institute of AstronomyKatholieke Universiteit LeuvenLeuvenBelgium
  2. 2.Departement Astrofysica, IMAPPRadboud Universiteit NijmegenNijmegenThe Netherlands
  3. 3.Nordic Optical TelescopeSanta Cruz de la PalmaSpain
  4. 4.Dr. Remeis-SternwarteUniversität Erlangen-NürnbergErlangenGermany

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