Orbit Orientation of the Planet in τ Boo (HD 120136)


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We determined the rotation period and the parameters of the global magnetic field of τ Boo. This allowed us to estimate the inclination of the rotational axis of the star to the line of sight, as well as to obtain estimates of the inclination of the planet’s orbital plane to the stellar equator.

作者简介

V. Bychkov

Special Astrophysical Observatory

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Email: vbych@sao.ru
俄罗斯联邦, Nizhnii Arkhyz, 369167

L. Bychkova

Special Astrophysical Observatory

Email: vbych@sao.ru
俄罗斯联邦, Nizhnii Arkhyz, 369167

G. Topilskaya

North-Caucasus Federal University

Email: vbych@sao.ru
俄罗斯联邦, Stavropol, 355017

J. Madey

Astronomical Observatory of the University of

Email: vbych@sao.ru
波兰, Warsaw, 00 011

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