A1 Refereed original research article in a scientific journal

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




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

PublisherEDP SCIENCES S A

Publication year2015

Journal: Astronomy and Astrophysics

Journal name in sourceASTRONOMY & ASTROPHYSICS

Journal acronymASTRON ASTROPHYS

Article numberARTN A84

Volume577

Number of pages5

ISSN0004-6361

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


Abstract

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.




Last updated on 26/11/2024 09:17:49 PM