No CrossRef data available.
Article contents
Some Remarks on the Unique Cepheid HR 7308
Published online by Cambridge University Press: 12 April 2016
Extract
HR 7308 is an apparently normal Pop. I Cepheid (Percy & Evans 1980; van Genderen 1981) with a constant period P = 1.49 days. However, its amplitude is variable with a range from about 5 to 20 km/sec in radial velocity and 0.05 to 0.30 in visual magnitude. The timescale for this variation is about 1200 days. According to Breger (1981) and Burki, et al. (1982; hereafter BMB), the star seems to be pulsating in a single modulated radial mode. Using published 0-values BMB identify this mode as a second or higher overtone. These authors also estimate a radius R = 34 ± 5 Rʘ and, based in part upon the observations of van Genderen (1981), a temperature log Te = 3.786 ± 0.01 and a gravity log g = 2.25 ± 0.25.
- Type
- Part I. Fundamental Parameters
- Information
- International Astronomical Union Colloquium , Volume 82: Cepheids: Theory and Observations , 1985 , pp. 93 - 94
- Copyright
- Copyright © Cambridge University Press 1985