Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Kalinicheva, E. S."'
Modeling the outflow of planetary atmospheres is important for understanding the evolution of exoplanet systems and for interpreting their observations. Modern theoretical models of exoplanet atmospheres become increasingly detailed and multicomponen
Externí odkaz:
http://arxiv.org/abs/2105.14343
Autor:
Kalinicheva, E. S.1 (AUTHOR) kalinicheva@inasan.ru, Shematovich, V. I.1 (AUTHOR), Savanov, I. S.1 (AUTHOR)
Publikováno v:
Astronomy Reports. Dec2022, Vol. 66 Issue 12, p1318-1324. 7p.
Autor:
Savanov, I. S.1 (AUTHOR) igs231@mail.ru, Kalinicheva, E. S.1 (AUTHOR), Dmitrienko, E. S.2 (AUTHOR)
Publikováno v:
Astrophysics. 2020, Vol. 63 Issue 4, p504-510. 7p.
Autor:
Shematovich, V. I.1 (AUTHOR) shematov@inasan.ru, Kalinicheva, E. S.1 (AUTHOR)
Publikováno v:
Astronomy Reports. Jul2020, Vol. 64 Issue 7, p628-635. 8p.
Publikováno v:
Astronomy Reports. May2018, Vol. 62 Issue 5, p352-358. 7p.
В данной работе представлены результаты моделирования верхней атмосферы экзопланеты π Men c, выполненные с помощью ранее разработанной о
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______917::5336e5d386999b29a853c2cea81c4a07
https://hdl.handle.net/10995/98954
https://hdl.handle.net/10995/98954
We used the previously developed self-consistent 1D model of hydrogen-helium atmosphere with suprathermal electrons accounted [1] to calculate the rate of close-in Naeptune atmospheric loss. The two-scale structure of the close-in (hot) Neptune atmos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______917::142c400a6c0c0b4d7868a4a2cee28feb
https://www.elibrary.ru/item.asp?id=42713847
https://www.elibrary.ru/item.asp?id=42713847
We present calculated periodograms and relative shear of possible differential rotators in Pleiades and Praesepe clusters. For some stars we are able to estimate inclinations roughly from theoretical predictions. По периодограммам з
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______917::9707b5419d512c9d92e82aad61664dc7
https://hdl.handle.net/10995/66781
https://hdl.handle.net/10995/66781
We present estimations of spottedness parameters S (the fraction of the visible surface of the star occupied by spots) of 674 stars in the Praesepe Cluster (age 650 Myr). Compared with parameters S of stars in the Pleiades Cluster (age 125 Myr) they
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______917::570787e127822da709beed62a9f52e06
https://elibrary.ru/item.asp?id=40116823
https://elibrary.ru/item.asp?id=40116823