Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.267.1103h&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Vol. 267, NO. 4/APR15, P.1103, 1994
Astronomy and Astrophysics
Astronomy
4
Stars: Early-Type Stars: Oscillations - Cepheids
Scientific paper
We have photometrically monitored nine intermediate- to high-Galactic-latitude B-type stars for β Cephei-type variability. One star, HD 204076, shows a clearly sinusoidal variation with an amplitude of 0.015 mag and a period of a few hours, typical of β Cephei stars. One other (HD 206144) is possibly a longer term variable at the 2 per cent level, while two objects, HD 219188 and HD 118246, may be variable at a smaller amplitude of < 0.0t mag. The remaining five stars show no signs of any periodic changes above 0.0t mag and are therefore unlikely to belong to the β Cephei class of variable.
Dufton Philip L.
Hambly Nigel C.
Keenan Francis P.
Kilkenny Dave
Marang Freddy
No associations
LandOfFree
A Search for Beta-Cephei Type Variability in a Sample of Intermediate Galactic Latitude to High Galactic Latitude B-Type Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A Search for Beta-Cephei Type Variability in a Sample of Intermediate Galactic Latitude to High Galactic Latitude B-Type Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Search for Beta-Cephei Type Variability in a Sample of Intermediate Galactic Latitude to High Galactic Latitude B-Type Stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1260407