Article (Scientific journals)
Asteroseismology of the β Cephei star KP Per
Saesen, S.; Briquet, Maryline; Cuypers, J. et al.
2007In Communications in Asteroseismology, 150, p. 197
Peer reviewed
 

Files


Full Text
2007CoAst.150..197S.pdf
Publisher postprint (135.91 kB)
Download

All documents in ORBi are protected by a user license.

Send to



Details



Abstract :
[en] We investigated the oscillations of the β Cephei star KP Per (HD 21803, B2IV, V=6.41) using Geneva photometry. We performed a detailed frequency analysis and a mode identification by means of photometric amplitude ratios. Then we confronted our deduced observational oscillation spectrum with that predicted by theory in order to determine a range for some stellar parameters, such as the mass and radius of KP Per.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Saesen, S.
Briquet, Maryline ;  KULeuven > Institut voor Sterrenkunde
Cuypers, J.
De Cat, P.
Goossens, K.
Language :
English
Title :
Asteroseismology of the β Cephei star KP Per
Publication date :
01 June 2007
Journal title :
Communications in Asteroseismology
ISSN :
1021-2043
eISSN :
2224-8374
Publisher :
Verlag der Österreichischen Akademie der Wissenschaften, Wien, Austria
Volume :
150
Pages :
197
Peer reviewed :
Peer reviewed
Available on ORBi :
since 20 June 2012

Statistics


Number of views
19 (0 by ULiège)
Number of downloads
26 (0 by ULiège)

OpenCitations
 
0

Bibliography


Similar publications



Contact ORBi