Optical flares on the RS CVn binary II Peg.
Abstract
During 57.4 hr of optical monitoring in the Johnson U- and B-bands of the RS CVn binary II Peg, 10 flares were detected. The absolute energies of these events are in the range 1-180 x 10 exp 33 erg. This implies a flare activity in the U-band of 0.17 flares per hour, compared with 0.12 flares per hour from UV C IV data. A double power-law distribution is required to fit the cumulative flare-frequency distribution of the U-band flares.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- March 1992
- DOI:
- 10.1093/mnras/255.1.48
- Bibcode:
- 1992MNRAS.255...48M
- Keywords:
-
- Binary Stars;
- Chromosphere;
- Giant Stars;
- K Stars;
- Main Sequence Stars;
- Stellar Flares;
- Frequency Distribution;
- Iue;
- Stellar Coronas;
- Stellar Spectra;
- Subgiant Stars;
- Astrophysics