Please use this identifier to cite or link to this item: https://dspace.ncfu.ru/handle/20.500.12258/3575
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dc.contributor.authorTopilskaya, G. P.-
dc.contributor.authorТопильская, Г. П.-
dc.date.accessioned2018-12-11T08:56:21Z-
dc.date.available2018-12-11T08:56:21Z-
dc.date.issued2018-
dc.identifier.citationBychkov, V.D., Bychkova, L.V., Topilskaya, G.P., Madey, J. Orbit Orientation of the Planet in τ Boo (HD 120136) // Astrophysical Bulletin. - 2018. - Volume 73. - Issue 4. - Pages 466-470ru
dc.identifier.urihttps://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=-
dc.identifier.urihttp://hdl.handle.net/20.500.12258/3575-
dc.description.abstractWe 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 equatorru
dc.language.isoenru
dc.publisherPleiades Publishingru
dc.relation.ispartofseriesAstrophysical Bulletin-
dc.subjectT Booru
dc.subjectMagnetic fieldru
dc.subjectPlanetary systemru
dc.titleOrbit prientation of the planet in τ Boo (HD 120136)ru
dc.typeСтатьяru
vkr.amountPages 466-470ru
vkr.instИнститут математики и естественных наук-
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