On the use of the Fourier transform to determine the projected rotational velocity of line-profile variable B stars⋆
Publication year
2014Source
Astronomy and Astrophysics, 569, (2014), article A118ISSN
Publication type
Article / Letter to editor

Display more detailsDisplay less details
Organization
Astrophysics
Journal title
Astronomy and Astrophysics
Volume
vol. 569
Subject
AstronomyThis item appears in the following Collection(s)
- Academic publications [204968]
- Electronic publications [103216]
- Faculty of Science [32332]
- Open Access publications [71771]
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.