B, V photometry of the active RS CVn system II Peg

Details B, V photometry of the active RS CVn system II Peg B, V photometry of the active RS CVn system II Peg

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.143..123e&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 143, no. 1, April 1988, p. 123-136.

Astronomy and Astrophysics

Astrophysics

4

Astronomical Photometry, Binary Stars, Light Curve, Pre-Main Sequence Stars, Stellar Activity, Variable Stars, Signal To Noise Ratios, Stellar Evolution, Ubv Spectra

Scientific paper

In this work, B and V photometry of the RS CVn-type binary II Peg is
presented. The light curves obtained in 1983 and 1984 display two
unequal maxima. The light curves of the system have different
amplitudes. The amplitude seems to vary with three different periods.
10, 6 and 4 years of periods may be attributed to those variations.

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