A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä

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




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

KustantajaEDP SCIENCES S A

Julkaisuvuosi2015

Lehti: Astronomy and Astrophysics

Tietokannassa oleva lehden nimiASTRONOMY & ASTROPHYSICS

Lehden akronyymiASTRON ASTROPHYS

Artikkelin numeroARTN A84

Vuosikerta577

Sivujen määrä5

ISSN0004-6361

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


Tiivistelmä

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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