Joan edukira

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

Gorde:
Xehetasun bibliografikoak
Egile Nagusiak: Topilskaya, G. P., Топильская, Г. П.
Formatua: Статья
Hizkuntza:English
Argitaratua: Pleiades Publishing 2018
Gaiak:
Sarrera elektronikoa: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
Etiketak: Etiketa erantsi
Etiketarik gabe, Izan zaitez lehena erregistro honi etiketa jartzen!