Zobrazeno 1 - 10
of 51
pro vyhledávání: '"Yuri Shchekinov"'
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 1, p 26 (2024)
The recent detection of large column density absorption lines from highly ionized gas in a few directions through the circumgalactic medium (CGM) of the Milky Way (MW) has been puzzling. The inferred temperature from these absorption lines far exceed
Externí odkaz:
https://doaj.org/article/a892537d0a564aa9b673f225d867e4c3
Autor:
Yuri Shchekinov
Publikováno v:
Galaxies, Vol 6, Iss 2, p 62 (2018)
The article aims to overview the origin and current dynamical state of a giant structure on the northern galactic sky—the radio Loop I extending from ≈ − 45 ∘ to ≈ + 45 ∘ in longitudes and up to ≈ 80 ∘ in latitudes over the Galactic c
Externí odkaz:
https://doaj.org/article/922f1f03ac1243f9ac58f0d2c89e131a
Publikováno v:
Proceedings of The Multifaceted Universe: Theory and Observations - 2022 — PoS(MUTO2022).
Autor:
Thijs de Graauw, Dmitry Novikov, A. S. Andrianov, Anton Vasyunin, Igor Zinchenko, A. O. Lyakhovets, Igor D. Novikov, Andrey Smirnov, D. Wiebe, S. F. Likhachev, Aleksey Georgievich Rudnitsky, Yuri Shchekinov, L. N. Likhacheva, V. I. Shematovich, T. I. Larchenkova, Anna Punanova, V. I. Kostenko, A. G. Doroshkevich, Sergei Vladimirovich Pilipenko, Andrey M. Baryshev, Nikolai S. Kardashev
Publikováno v:
Physics Uspekhi, 64(4), 386-419
Physics-Uspekhi
Physics-Uspekhi
We present the scientific program of the Spectr-M project aimed at the creation and operation of the Millimetron Space Observatory (MSO) planned for launch in the late 2020s. The unique technical capabilities of the observatory will enable broadband
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff59500a3fa21bd8e855eb2ee309ef66
https://research.rug.nl/en/publications/495be66c-7e2d-4604-859d-2f48a0d339a4
https://research.rug.nl/en/publications/495be66c-7e2d-4604-859d-2f48a0d339a4
Autor:
V. I. Shematovich, Thijs de Graauw, Dmitry Novikov, A. G. Doroshkevich, Anton Vasyunin, Andrey Smirnov, Sergei Vladimirovich Pilipenko, T. I. Larchenkova, Anna Punanova, S. F. Likhachev, Nikolai S. Kardashev, A. S. Andrianov, Yuri Shchekinov, V. I. Kostenko, Aleksey Georgievich Rudnitsky, Igor Zinchenko, D. Wiebe, Andrey M. Baryshev, A. O. Lyakhovets, Igor D. Novikov, L. N. Likhacheva
Publikováno v:
Uspekhi Fizicheskih Nauk. 191
Publikováno v:
Universe. 8:212
The presence of dust in the intracluster medium (ICM) has been a long-standing problem that is still awaiting elucidation. Direct observational diagnostics are rather challenging (though not impossible) either because of a sparse distribution of dust
Autor:
V. A. Ladygin, Volodymyr Kudriashov, A. G. Rudnitskiy, V. I. Kostenko, Yuri Shchekinov, Heino Falcke, Freek Roelofs, A. R. Shaykhutdinov, I. A. Girin, T. de Graauw, A. S. Andrianov, S. F. Likhachev, Andrey M. Baryshev, M. A. Shchurov
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 500(4), 4866-4877. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 500, 4866-4877
Monthly Notices of the Royal Astronomical Society, 500, 4, pp. 4866-4877
Monthly Notices of the Royal Astronomical Society, 500, 4866-4877
Monthly Notices of the Royal Astronomical Society, 500, 4, pp. 4866-4877
High resolution imaging of supermassive black holes shadows is a direct way to verify the theory of general relativity at extreme gravity conditions. Very Long Baseline Interferometry (VLBI) observations at millimeter/sub-millimeter wavelengths can p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::df0664f93798c6196c932abfc1688907
http://arxiv.org/abs/2006.10120
http://arxiv.org/abs/2006.10120
Publikováno v:
Open Astronomy, Vol 27, Iss 1, Pp 1-6 (2018)
In this paper, we address the question of how a central intermediate-mass black hole (IMBH) in a globular cluster (GC) affects dynamics, core collapse, and formation of the binary population. It is shown that the central IMBH forms a binary system th
Publikováno v:
Open Astronomy, Vol 26, Iss 1, Pp 224-232 (2017)
Using 3-D gas dynamic simulations, we study the supernova (SNe) driven transport of gas from the galactic disk. We assume that SNe are distributed randomly and uniformly in the galactic plane and we consider sufficiently high volume SNe rates that ar
Publikováno v:
Physics-Uspekhi. 60:961-993