Rotation and activity of young late-type stars: Optical variability of eight weak-line T Tauri stars during 1992-1995

Details Rotation and activity of young late-type stars: Optical variability of eight weak-line T Tauri stars during 1992-1995 Rotation and activity of young late-type stars: Optical variability of eight weak-line T Tauri stars during 1992-1995

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997astl...23..615g&link_type=abstract

Astronomy Letters, Volume 23, Issue 5, September 1997, pp.615-622; Pis'ma v Astronomicheskii Zhurnal, Vol. 23, p. 700

Astronomy and Astrophysics

Astronomy

Scientific paper

The photoelectric BVR photometry of eight weak-line T Tauri stars that was performed during 1992-1995 is presented. All of the stars exhibit periodic light variations attributable to cool photospheric spots. The photometric periods range from 0.7 to 10 days. For all these stars, the positions are shown in the two-color B-V, V-R diagram. Changes in the amplitude and shape of the folded light curves are discussed.

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