Publication year
2007Source
Communications in Asteroseismology, 150, (2007), pp. 189-190ISSN
Publication type
Article / Letter to editor
Display more detailsDisplay less details
Organization
Astrophysics
Journal title
Communications in Asteroseismology
Volume
vol. 150
Page start
p. 189
Page end
p. 190
Subject
AstronomyAbstract
We report results from mode identifications (MI) for four selected multi-periodic Slowly Pulsating B-stars (SPB) using the Fourier parameter fit (FPF) method. Problems related to the pulsational nature of these objects which hamper a correct identification are discussed. For a present day status of knowledge about SPB stars we refer to De Cat (2007, this issue).
This item appears in the following Collection(s)
- Academic publications [245131]
- Electronic publications [132467]
- Faculty of Science [37407]
- Open Access publications [106066]
Upload full text
Use your RU credentials (u/z-number and password) to log in with SURFconext to upload a file for processing by the repository team.