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Orbit prientation of the planet in τ Boo (HD 120136)

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

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Detaylı Bibliyografya
Asıl Yazarlar: Topilskaya, G. P., Топильская, Г. П.
Materyal Türü: Статья
Dil:English
Baskı/Yayın Bilgisi: Pleiades Publishing 2018
Konular:
Online Erişim:https://www.scopus.com/record/display.uri?eid=2-s2.0-85057442199&origin=resultslist&sort=plf-f&src=s&nlo=&nlr=&nls=&sid=e1e93e1e7183319c023a8801b2755338&sot=aff&sdt=sisr&sl=174&s=AF-ID%28%22North+Caucasus+Federal+University%22+60070541%29+OR+AF-ID%28%22Stavropol+State+University%22+60070961%29+OR+AF-ID%28%22stavropolskij+Gosudarstvennyj+Tehniceskij+Universitet%22+60026323%29&ref=%28Orbit+Orientation+of+the+Planet+in+%CF%84+Boo%29&relpos=0&citeCnt=0&searchTerm=
https://dspace.ncfu.ru/handle/20.500.12258/3575
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