Zobrazeno 1 - 10
of 13
pro vyhledávání: '"S. V. Salii"'
Autor:
S. V. Salii
Publikováno v:
Астрономия и исследование космического пространства: Всероссийская с международным участием научная конференция студентов и молодых ученых, посвященная памяти Полины Евгеньевны Захаровой.
The physical conditions were estimated from the methanol radio lines observed at 0.8 mm with IRAM30m in the star-forming region S255IR-SMA1. In the approximation of a large velocity gradient (LVG), the values of the gas kinetic temperature (170 K), t
Publikováno v:
Астрономия и исследование космического пространства: Всероссийская с международным участием научная конференция студентов и молодых ученых, посвященная памяти Полины Евгеньевны Захаровой.
The article is dedicated to the memory of Polina Evgenievna Zakharova (12.03.1940—28.09.2020), our Teacher, stellar astronomer, Candidate of Science in Physics and Mathematics, director of the Kourovka Astronomical Observatory of the Ural Universit
Autor:
A. M. Sobolev, S. V. Salii
Publikováno v:
Proceedings of the 48-th International student's conferences "Physics of Space".
Autor:
S. V. Salii, A. P. Shevelev
Publikováno v:
Proceedings of the 48-th International student's conferences "Physics of Space".
Работа поддержана Министерством науки РФ, базовая часть госзадания, РК № AAAA-A17-117030310283-7, и Правительством РФ, контракт № 02.A03.21.0006, постано
Publikováno v:
Astron. Rep.
Astronomy Reports
Astronomy Reports
The results of a detailed analysis of SMA, VLA, and IRAM observations of the region of massive star formation S255N in CO(2---1), \nh, \nhh, \co and some other lines is presented. Combining interferometer and single-dish data has enabled a more detai
Autor:
Y. Wang, Igor Zinchenko, Devendra K. Ojha, S. V. Salii, Henrik Beuther, Sheng-Yuan Liu, P. M. Zemlyanukha, Andrej M. Sobolev, Yu-Nung Su, Manash R. Samal
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2015, 810 (1), ⟨10.1088/0004-637X/810/1/10⟩
The Astrophysical Journal, American Astronomical Society, 2015, 810 (1), ⟨10.1088/0004-637X/810/1/10⟩
Astrophysical Journal
Astrophysical Journal, American Astronomical Society, 2015, 810 (1), 〈10.1088/0004-637X/810/1/10〉
The Astrophysical Journal, 2015, 810 (1), ⟨10.1088/0004-637X/810/1/10⟩
The Astrophysical Journal, American Astronomical Society, 2015, 810 (1), ⟨10.1088/0004-637X/810/1/10⟩
Astrophysical Journal
Astrophysical Journal, American Astronomical Society, 2015, 810 (1), 〈10.1088/0004-637X/810/1/10〉
We report the results of our observations of the S255IR area with the SMA at 1.3 mm in the very extended configuration and at 0.8 mm in the compact configuration as well as with the IRAM-30m at 0.8 mm. The best achieved angular resolution is about 0.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6a2a2c9da4430451391dc72f44195ee1
https://hal.science/hal-01441190
https://hal.science/hal-01441190
Autor:
A. M. Sobolev, S. V. Salii
Publikováno v:
Astronomy Reports. 50:965-982
The results of SEST millimeter observations of the molecular cloud G345.01+1.79 are presented. Spectra of CH3OH, SO2, SiO, HCO+, C18O, C33S, C34S, HCN, and DCN lines have been obtained. Mapping of the cloud in CH3OH, SiO, and C34S lines indicates tha
Autor:
S. V. Salii, E. C. Sutton, L. E. B. Johansson, Simon Ellingsen, Igor Zinchenko, A. M. Sobolev
Publikováno v:
Astronomical & Astrophysical Transactions. 22:7-10
We report molecular line observations of the G34.26+0.15/34.24+0.13 complex, which contains a bright molecular core and a proto-B-star. ATCA observations show that both objects are closely associated with 6.7 v GHz class II methanol masers. Methanol
Publikováno v:
Astronomy Reports. 46:955-968
Observations of the molecular cloud G1.6-0.025 in the 2K-1K and J0-J−1E series and 5−1-40E line of CH3OH, the (2-1) and (3-2) lines of SiO, and the 7−7-6−6 line of HNCO are described. Maps of the previously observed extended cloud with Vlsr
Publikováno v:
Astrophysical Journal
We present the results of an interferometric study of 38 millimeter-wave lines of CH3OH in the region around the water maser source W3(H2O) and a region extending about 30" to the south and west of the hydroxyl maser source W3(OH). The methanol emitt
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::46a19bb3eac2ba54787cf88341096ec9
https://hdl.handle.net/10995/73099
https://hdl.handle.net/10995/73099