Periodicity in some light curves of the solar analogue V352 Canis Majoris




Kajatkari P, Jetsu L, Cole E, Hackman T, Henry GW, Joutsiniemi SL, Lehtinen J, Makela V, Porceddu S, Ryynanen K, Solea V

2015

 Astronomy and Astrophysics

ASTRONOMY & ASTROPHYSICS

ASTRON ASTROPHYS

ARTN A84

577

5

0004-6361

DOIhttps://doi.org/10.1051/0004-6361/201322847



Results. We found an apparent 11.7 +/- 0.5 yr cycle in the mean brightness. The mean of the individual photometric rotation periods is 7.24 +/- 0.22 days. The lower limit for the differential rotation coefficient is vertical bar k vertical bar > 0.12, assuming that period changes in V352 CMa follow the solar pattern. The Kuiper method detected stable, active longitudes rotating with a period of 7.157 +/- 0.002 days, from the epochs of light minimum, but these structures vanished after the year 2009. CPS performed better than the traditional PSM, because the latter assumes a sinusoidal model for the data even when this was not correct.




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