Zobrazeno 1 - 7
of 7
pro vyhledávání: '"S. Y. Zubrin"'
Autor:
O. M. Patoka, V. M. Shulga, O. V. Antyufeyev, S. Y. Zubrin, V. V. Myshenko, A. M. Korolev, V. I. Piddyachiy
Publikováno v:
Radio Physics and Radio Astronomy, Vol 22, Iss 3, Pp 173-200 (2017)
Purpose: The statistical features of emission in CS (J = 2 - 1) line, Class II methanol masers and IR sources in the regions associated with the Class II methanol masers are studied. Design/methodology/approach: The survey is performed at the CS (
Externí odkaz:
https://doaj.org/article/b99576db9a84456db1194b2205493e2f
Autor:
V. M. Shulga, O. V. Antyufeyev, S. Y. Zubrin, V. V. Myshenko, V. I. Piddyachiy, A. M. Korolev, O. M. Patoka
Publikováno v:
Radio Physics and Radio Astronomy, Vol 22, Iss 2, Pp 112-122 (2017)
Purpose: Some peculiarities of emission of Class I methanol masers on the 80–71A+ transition at 95 GHz in sources closely associated with protostar-forming regions and in supernova remnants are studied. Here belongs the investigation of SiO (J=2–
Externí odkaz:
https://doaj.org/article/33184a7c79724a998b392691a0618304
Autor:
O. M. Patoka, Oleksandr Antyufeyev, V. M. Shulga, A. M. Korolev, V. V. Myshenko, S. Y. Zubrin, V. I. Piddyachiy
Publikováno v:
Radio Physics and Radio Astronomy, Vol 22, Iss 2, Pp 112-122 (2017)
Purpose: Some peculiarities of emission of Class I methanol masers on the 80–71A+ transition at 95 GHz in sources closely associated with protostar-forming regions and in supernova remnants are studied. Here belongs the investigation of SiO (J=2–
Publikováno v:
Radio Physics and Radio Astronomy. 3:19-26
Autor:
V. I. Shkodin, A. V. Poladich, A. M. Korol, V. V. Myshenko, A. V. Antyufeyev, O. M. Korolev, S. Y. Zubrin, V. M. Shulga, V. I. Piddyachiy
Publikováno v:
Radio Physics and Radio Astronomy. 2:99-104
Autor:
V. V. Myshenko, V. I. Piddyachiy, A. V. Antyufeev, S. Y. Zubrin, V. M. Shulga, A. V. Myshenko, A. M. Korolev
Publikováno v:
2006 16th International Crimean Microwave and Telecommunication Technology.
Low noise cryogenic microwave spectrometer (MS) for 85...115 GHz band is suggested for cosmic maser lines observations on RT-22 with high spectral resolution. Provided are the results of observations of certain space masers.
Autor:
Patoka, O. M., Shulga, V. M., Antyufeyev, O. V., Myshenko, V. V., Korolev, A. M., Piddyachiy, V. I.
Publikováno v:
Kinematics & Physics of Celestial Bodies; Sep2018, Vol. 34 Issue 5, p217-257, 41p