Article (Scientific journals)
Synthetic pulsational line profile variations
Oreiro, R.; Telting, J. H.; Østensen, R. H. et al.
2010In Astrophysics and Space Science, 329, p. 211-216
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Keywords :
Asteroseismology; Hot subdwarfs
Abstract :
[en] 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.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Oreiro, R.;  Institute of Astronomy, Katholieke Universiteit Leuven
Telting, J. H.;  Nordic Optical Telescope
Østensen, R. H.;  Institute of Astronomy, Katholieke Universiteit Leuven
Briquet, Maryline ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Aerts, C.;  Institute of Astronomy, Katholieke Universiteit Leuven ; Departement Astrofysica, IMAPP, Radboud Universiteit Nijmegen
Heber, U.;  Dr. Remeis-Sternwarte, Universität Erlangen-Nürnberg
Vučković, M.;  Institute of Astronomy, Katholieke Universiteit Leuven
Language :
English
Title :
Synthetic pulsational line profile variations
Publication date :
01 October 2010
Journal title :
Astrophysics and Space Science
ISSN :
0004-640X
eISSN :
1572-946X
Publisher :
Springer Science & Business Media B.V., Dordrecht, Netherlands
Volume :
329
Pages :
211-216
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 28 January 2013

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