MOST Photometry of the roAp star HD 134214

Author(s)
Chris Cameron, Jaymie M. Matthews, Rainer Kuschnig, Werner Wolfgang Weiss
Abstract

We present 10.27 hrs of photometry of the roAp star HD 134214 obtained by the MOST1 satellite. The star is shown to be monoperiodic and oscillating at a frequency of 2948.97 ± 0.55 ?Hz. This is consistent with earlier ground based photometric campaigns (e.g. Kreidl et al. 1994). We do not detect any of the additional frequencies identified in the recent spectroscopic study by Kurtz et al. (2006) down to an amplitude limit of 0.36 mmag (2? significance limit).

Organisation(s)
Department of Astrophysics
External organisation(s)
University of British Columbia (UBC)
Journal
Communications in Asteroseismology
Volume
148
Pages
57-64
No. of pages
8
ISSN
1021-2043
DOI
https://doi.org/10.1553/cia148s57
Publication date
2006
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy
Portal url
https://ucrisportal.univie.ac.at/en/publications/9ff91002-9e01-4f6c-887d-66d476f5c5bc