Light curve analysis for RY Tau

Details Light curve analysis for RY Tau Light curve analysis for RY Tau

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012arep...56..131i&link_type=abstract

Astronomy Reports, Volume 56, Issue 2, pp.131-137

Astronomy and Astrophysics

Astronomy

Scientific paper

We have analyzed a master light curve of the classical T Tauri star RY Tau. The brightness variations observed in 1983-2004 were found to be periodic. A period of 377 ± 10 d is derived using a frequency analysis. A statistical analysis shows that the brightness variability cannot be described by a normal distribution. The brightness variations could be due to the presence of some bodies being formed in the circumstellar environment.

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