Bibcode
Lazaro, C.; Arévalo, M. J.
Bibliographical reference
Activity in cool star envelopes, p. 111 - 114
Advertised on:
0
1988
Citations
0
Refereed citations
0
Description
Infrared and V band photometry of the RS CVn system II Peg, carried out
in 1984 and 1986, has been analysed with a simple model in order to
follow the evolution of the activity of spots over the surface of the
visible star. The group of spots has been concentrated in longitude from
1984 to 1986 covering about 27% in 1984 and 44% of the visible disk in
1986. During both observation periods, the system shows an IR excess too
high to be attributable to the presence of spots and the authors suggest
it to be caused by dust around the system.