The active radio star HD 36705.
Abstract
The present paper describes a concentrated series of observations that were made at 8.4 GHz in December 1985 and January/February 1986. Observations of this star are important because it differs from the active stars in RS CVn binaries in being a rapidly rotating single star with the spectrum and colour indices of a normal G8 V star. The aim of the experiment was to investigate the flux and polarization variability over several rotations of the star during flare activity.
- Publication:
-
Publications of the Astronomical Society of Australia
- Pub Date:
- 1986
- DOI:
- 10.1017/S132335800002693X
- Bibcode:
- 1986PASA....6..312S
- Keywords:
-
- Radiant Flux Density;
- Radio Stars;
- Stellar Activity;
- Stellar Coronas;
- Stellar Spectrophotometry;
- Circular Polarization;
- Spectral Energy Distribution;
- Starspots;
- Stellar Temperature;
- Synchrotron Radiation;
- Astrophysics;
- Radio Flares:Radio Stars;
- Radio Stars:Radio Flares