New 'flip-flop' of FK Comae Berenices

Details New 'flip-flop' of FK Comae Berenices New 'flip-flop' of FK Comae Berenices

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...282l...9j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 282, no. 1, p. L9-L12

Astronomy and Astrophysics

Astrophysics

18

Ephemerides, Giant Stars, Stellar Magnitude, Stellar Mass, Stellar Spectrophotometry, Variable Stars, Light Curve, Spectroscopic Telescopes, Stellar Rotation

Scientific paper

New UBVR photometry of FK Comae Berenices shows that the concentrated
part of the spot distribution has shifted to a new active longitude,
which is consistent with the recently defined 'flip-flop' ephemeris for
a quarter of a century of photometry. The new 'flip-flop' of FK Comae
Berenices is the fourth one detected during 26.3 years.

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