Zobrazeno 1 - 10
of 26
pro vyhledávání: '"S. Yu. Gorda"'
Autor:
M. A. Pogodin, S. E. Pavlovskii, N. G. Beskrovnaya, N. A. Drake, O. V. Kozlova, I. Yu. Alekseev, M. Borges Fenandes, C. B. Pereira, G. G. Valyavin, A. S. Miroshnichenko, S Yu. Gorda, D. L. Gorshanov
Publikováno v:
Astrophysics. 65:31-52
Autor:
S. Yu. Gorda
Publikováno v:
Astronomy Reports. 64:922-935
The results of 14-year photometric monitoring of the contact close binary system (CBS) W UMa-type AM Leo are presented. Low-amplitude cyclic variations in brightness with a period of $$7.6 \pm 0.3$$ years, not associated with the phenomena of eclipse
Autor:
S. Yu. Gorda
Publikováno v:
Астрономия и исследование космического пространства: Всероссийская с международным участием научная конференция студентов и молодых ученых, посвященная памяти Полины Евгеньевны Захаровой.
Based on the 14-year photometric CCD monitoring of the contact eclipsing variable star AM Leo of type W UMa carried out author from 2007 to 2020 at the telescopes of the Kourovka observatory UrFU, the presence cyclic variations in brightness of the s
Planets are thought to form at the early stage of stellar evolution when the mass accretion is still ongoing. RY Tau is a T Tauri type star at the age of a few Myr, with accretion disc seen at high inclination, so that line of sight crosses both the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0a26d03c04f72dff0521a99ab94b8a31
Autor:
Y. Yu. Vatolin, S. Yu. Gorda
Publikováno v:
Proceedings of the 48-th International student's conferences "Physics of Space".
Autor:
S. Yu. Gorda, T. S. Polushina
Publikováno v:
Proceedings of the 48-th International student's conferences "Physics of Space".
Autor:
S. Yu. Gorda
Publikováno v:
Astrophysical Bulletin. 72:321-329
This paper reports the results of spectroscopic observations of UUCas obtained with the highresolution (R = 15 000) fiber-fed echelle spectrometer of the 1.2-m telescope of Kourovka Astronomical Observatory of Ural Federal University. The radial velo
Autor:
Gösta F. Gahm, K. N. Grankin, A. A. Djupvik, T. R. Irsmambetova, P. P. Petrov, V. I. Shenavrin, S. A. Artemenko, E. V. Babina, J. F. Gameiro, David Mkrtichian, R. M. G. de Albuquerque, M. Fernandez, S. Yu. Gorda
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Mon. Not. R. Astron. Soc.
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 483 (1), pp.132-146. ⟨10.1093/mnras/sty3066⟩
instname
Mon. Not. R. Astron. Soc.
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 483 (1), pp.132-146. ⟨10.1093/mnras/sty3066⟩
Classical T Tauri stars with ages of less than 10 Myr possess accretion discs. Magnetohydro-dynamic processes at the boundary between the disc and the stellar magnetosphere control the accretion and ejections gas flows. We carried out a long series o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4783d94db2f4d8950d4b0214ac7236d4
http://hdl.handle.net/10261/189369
http://hdl.handle.net/10261/189369
Autor:
K. A. Antonyuk, S. P. Belan, N. V. Pit, N. I. Bondar, Yu. V. Pakhomov, V. I. Shenavrin, S. Yu. Gorda
Publikováno v:
Astron. Lett.
Astronomy Letters
Astronomy Letters
Based on the multiband (BVRIJHKL) photometric observations of the active red giant PZ Mon performed for the first time in the winter season of 2017-2018, we have determined the main characteristics of the spotted stellar surface in a parametric three
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f0b7a1b967dc0ba4c4f5a8367388c9c
Autor:
S. Yu. Gorda
Publikováno v:
Astronomy Letters. 42:693-702
We present the results of the reduction of our observations for the spectroscopic binary ADS 2984A (B0 II–B0 III), which along with its visual component ADS 2984B (SZ Cam) are the brightest members of the open star cluster NGC 1502. The spectroscop