Reference : A new version of the moment method, optimized for mode identification in multiperiodic s...
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/132474
A new version of the moment method, optimized for mode identification in multiperiodic stars
English
Briquet, Maryline mailto [KULeuven > Instituut voor Sterrenkunde > > >]
Aerts, C. [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium]
1-Feb-2003
Astronomy and Astrophysics
EDP Sciences
398
687-696
Yes (verified by ORBi)
International
0004-6361
1432-0746
Les Ulis
France
[en] line: profiles ; stars: oscillations ; stars: individual: beta Crucis ; 16 Lacertae ; HD 74195
[en] We present a numerical version of the moment method for the identification of non-radial pulsation modes. The new version requires less computation time than the previous one, allowing users to consider all the information contained in the first three moments of a multiperiodic star and to identify multiple modes simultaneously. This, together with the use of a new discriminant that considers the moments calculated at each time of observation, increases considerably the feasibility and the accuracy of the mode identification for multiperiodic stars. Moreover, the technique is extended to rotating pulsating stars. We apply the new version to three B stars showing multiperiodicity. Computer code for mode identification available upon request. Tables 1 to 8 are only available in electronic form at http://www.edpsciences.org
http://hdl.handle.net/2268/132474
also: http://hdl.handle.net/2268/140944
10.1051/0004-6361:20021683
http://esoads.eso.org/abs/2003A%26A...398..687B

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