A study of bright southern slowly pulsating B stars. II. The intrinsic frequencies
By P. Cat, C. Aerts. 2002
280 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/8dc5f5a2b25941c62d836492b9f31b4a86b4eafc
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In Astronomy and Astrophysics
In Atomic and Molecular Physics, and Optics
In Instrumentation
Citations in the corpus
- The orbit of the close spectroscopic binary ε Lup and the intrinsic variability of its early B-type components , (2005, background): “As the number of cases observed with confirmed tidally induced modes is sparse (HD 177 863, De Cat & Aerts 2002; HD 209 295, Handler et al. 2002), two complementary surveys have been set up to systematically study the behaviour of non-radial pulsations (NRPs) in early B-type stars with a close…”
- Probing the properties of convective cores through g modes : high-order g modes in SPB and γ Doradus stars (2008, methodology): “In addition to large observational efforts that have been made from the ground (see e.g. De Cat & Aerts 2002; De Cat et al. 2007 for SPB stars and Mathias et al. 2004; Henry, Fekel & Henry 2007 for γ Dor), long, uninterrupted space-based photometric time series will soon be provided by CoRoT.”
- Catalog of Galactic β Cephei Stars (2005, background): “For instance, the SPB stars are later type B stars (B2–B9) with light, radial velocity, and line profile variability with periods of the order of a few days (De Cat & Aerts 2002).”