On the variability of Sigma Geminorum - an interesting candidate for X-ray studies.
Abstract
Observations of Sigma Gem in UV show that high excitation line fluxes increase with the emergence of a dark region from behind the approaching limb. A moderate increase in X-ray intensity occurs, together with the coming into view of another, weaker, spot region. Further observations of rotational modulation effects are desirable.
- Publication:
-
Cosmic X-Ray Spectroscopy Mission
- Pub Date:
- September 1985
- Bibcode:
- 1985ESASP.239..117E
- Keywords:
-
- Binary Stars;
- Variable Stars;
- X Ray Astronomy;
- Stellar Rotation;
- Stellar Spectra;
- Ultraviolet Astronomy;
- Astronomy;
- RS CVn Stars:Starspots;
- RS CVn Stars:Stellar Activity;
- RS CVn Stars:UV Lines;
- RS CVn Stars:X Rays;
- Starspots:RS CVn Stars;
- Stellar Activity:RS CVn Stars;
- UV Lines:RS CVn Stars;
- X Rays:RS CVn Stars