On the benefits of photometry for roAp theory: MOST observations of γ Equulei (HD 201601)

Author(s)
Michael Gruberbauer, Werner Wolfgang Weiss
Abstract

We discuss the potential of space photometry for rapidly oscillating Ap (roAp) stars. In reference to the MOST observations of γ Equulei (Gruberbauer et al., 2008), we show that several aspects of the roAp phenomenon demand longer observational time bases and better time sampling than those currently feasible using spectroscopy. We conclude that, in order to improve our understanding of roAp stars, photometry is still an important tool which should not be neglected.

Organisation(s)
Department of Astrophysics
Journal
Contributions of the Astronomical Observatory Skalnaté Pleso
Volume
38
Pages
311-316
ISSN
1335-1842
Publication date
2008
Austrian Fields of Science 2012
103004 Astrophysics, 103003 Astronomy
Portal url
https://ucrisportal.univie.ac.at/en/publications/4462bb76-ddc8-452a-83fb-8f20e5b292d5