Article (Scientific journals)
Spectroscopic mode identification for the slowly pulsating B star HD 147394
Briquet, Maryline; Aerts, C.; Mathias, P. et al.
2003In Astronomy and Astrophysics, 401, p. 281-288
Peer Reviewed verified by ORBi
 

Files


Full Text
Briquet_2003.pdf
Publisher postprint (543.92 kB)
Download

All documents in ORBi are protected by a user license.

Send to



Details



Keywords :
line: profiles; stars: early-type; stars: oscillations; stars: rotation; stars: variables: general; stars: individual: HD 147394
Abstract :
[en] We present ground-based high-resolution high S/N spectra of the slowly pulsating B star HD 147394. Two frequencies are clearly found in the moments of the Si II 4128-4130 doublet: f[SUB]1[/SUB]=0.8008 c d[SUP]-1[/SUP] and f[SUB]2[/SUB]=0.7813 c d[SUP]-1[/SUP]. The frequency f[SUB]1[/SUB] is also found in the HIPPARCOS data. A third frequency is also present in our spectroscopic data: f[SUB]3[/SUB]=0.7175 c d[SUP]-1[/SUP] or its aliases due to the time sampling. A mode identification is performed by means of a new version of the moment method optimized for multiperiodic signals. It points towards several equivalent solutions of non-axisymmetric l <=3 for all three modes. We have too limited information to perform seismic modelling at this stage, but we do show that the different possibilities for the mode identifications are compatible with pulsational models for SPBs. Based on observations obtained with the spectrograph Aurélie attached to the 1.52-m telescope of the Observatoire de Haute-Provence, France.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Briquet, Maryline ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Aerts, C.;  Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, 3001 Leuven, Belgium
Mathias, P.;  Observatoire de la Côte d'Azur, Département Fresnel, UMR 6528, 06304 Nice Cedex 4, France
Scuflaire, Richard ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Evol. et stabilité des étoiles et des amas d'étoiles (ESEA)
Noels-Grötsch, Arlette ;  Institut d'Astrophysique et de Géophysique de Liège, Université de Liège, allée du Six Août 17, 4000 Liège, Belgium
Language :
English
Title :
Spectroscopic mode identification for the slowly pulsating B star HD 147394
Publication date :
01 April 2003
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP Sciences, Les Ulis, France
Volume :
401
Pages :
281-288
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 22 October 2012

Statistics


Number of views
44 (0 by ULiège)
Number of downloads
113 (0 by ULiège)

Scopus citations®
 
5
Scopus citations®
without self-citations
3
OpenCitations
 
3

Bibliography


Similar publications



Contact ORBi