Email this article Orbit Orientation of the Planet in τ Boo (HD 120136)
- Authors: Bychkov V.D.1, Bychkova L.V.1, Topilskaya G.P.2, Madey J.3
-
Affiliations:
- Special Astrophysical Observatory
- North-Caucasus Federal University
- Astronomical Observatory of the University of
- Issue: Vol 73, No 4 (2018)
- Pages: 466-470
- Section: Article
- URL: https://journal-vniispk.ru/1990-3413/article/view/212801
- DOI: https://doi.org/10.1134/S1990341318040090
- ID: 212801
Cite item
Open Access
Access granted
Subscription Access
Abstract
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.
About the authors
V. D. Bychkov
Special Astrophysical Observatory
Author for correspondence.
Email: vbych@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167
L. V. Bychkova
Special Astrophysical Observatory
Email: vbych@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167
G. P. Topilskaya
North-Caucasus Federal University
Email: vbych@sao.ru
Russian Federation, Stavropol, 355017
J. Madey
Astronomical Observatory of the University of
Email: vbych@sao.ru
Poland, Warsaw, 00 011
Supplementary files
