Rapid orbital precession of the eclipsing binary HS Hydrae
Azizbek MatekovUlugh Beg Astronomical Institute of the Uzbekistan Academy of Science, 33 Astronomicheskaya, Tashkent 100052, UzbekistanA. S. HojaevUlugh Beg Astronomical Institute of the Uzbekistan Academy of Science, 33 Astronomicheskaya, Tashkent 100052, Uzbekistan
ABI
Аннотация
Abstract We investigated the evolution of HS Hya system’s inclination based on analysis of its light curves in the period 1964–2021. HS Hya is EA type eclipsing binary star, belonging to separate group with changing orbital inclination. We used our recent observations as well as the data from sky surveys.
Мавзулар
Идентификаторлар
Иқтибослар ва манбалар
0 та иқтибос0 та фойдаланилган манба
Кўрсаткичлар — AkademScholar · Тез орада