Detection of rotation modulation in Rho OPH dark cloud T Tauri stars

Details Detection of rotation modulation in Rho OPH dark cloud T Tauri stars Detection of rotation modulation in Rho OPH dark cloud T Tauri stars

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17...50b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, Jan. 1991, p. 50-59. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

3

Dark Matter, Ophiuchi Clouds, Stellar Rotation, T Tauri Stars, Velocity Modulation, Brightness Distribution, Fourier Analysis, Light Curve, Variability

Scientific paper

Brightness curves for nine T Tauri stars in the Rho Oph dark cloud are
studied by Fourier analysis. A periodic component is found for five
stars: Haro 1-1, Haro 1-8, Haro 1-14, S-R 9 and V2058 Oph show a
periodic variability with periods of 3.35, 14.58, 8.20, 6.54 and 6.90,
respectively.

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