Zobrazeno 1 - 10
of 20
pro vyhledávání: '"V. I. Piddyachiy"'
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
Publikováno v:
Radio Physics and Radio Astronomy, Vol 20, Iss 3, Pp 261-268 (2015)
A low-noise uncooled receiver was designed and constructed for measurements of the atmospheric ozone spectral line at 142.2 GHz. The design has shown the double-sideband (DSB) receiver noise temperature of about 350 K within 130 to 150 GHz. Critical
Externí odkaz:
https://doaj.org/article/efdd6a8a46384812909f72d99c87e342
Autor:
V. I. Piddyachiy
Publikováno v:
Radio Physics and Radio Astronomy, Vol 20, Iss 1, Pp 86-93 (2015)
A Schottky diode frequency tripler for the 3-mm receiver system designed for observation of ozone and carbon monoxide spectral lines at frequencies 110.836 and 115.271 GHz, respectively, is developed. The used varactor parameters are investigated and
Externí odkaz:
https://doaj.org/article/f621d61aee304ba680cae328475d7f62
Publikováno v:
Kinematika i fizika nebesnyh tel (Online). 34:3-51
Autor:
O. M. Patoka, A. M. Korolev, Oleksandr Antyufeyev, V. I. Piddyachiy, V. M. Shulga, V. V. Myshenko
Publikováno v:
Kinematics and Physics of Celestial Bodies. 34:217-257
The paper aims at establishing relations between the parameters of methanol maser emission that originates in dense star-forming regions and parameters of a dense core using emission of the CS molecule. A total of 164 sources toward the positions of
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, Vol 20, Iss 3, Pp 261-268 (2015)
A low-noise uncooled receiver was designed and constructed for measurements of the atmospheric ozone spectral line at 142.2 GHz. The design has shown the double-sideband (DSB) receiver noise temperature of about 350 K within 130 to 150 GHz. Critical
Publikováno v:
Journal of Molecular Spectroscopy. :33-37
We present a new study of the millimeter wave spectrum of the lowest two conformers of the 1,3-propanediol (CH2OHCH2CH2OH) molecule. The new measurements involving rotational transitions with J up to 65 and Ka up to 30 for conformer I and J up to 59
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