Zobrazeno 1 - 10
of 279
pro vyhledávání: '"M. A. Pashchenko"'
Publikováno v:
Applied Mathematics and Control Sciences. :45-66
Mathematical modeling of the deformation behavior of a Panda-type optical fiber with protective and hardening coatings was performed as part of the work. The contact indentation of a fiber into in aluminum half-space is simulated. The different patte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4cd993bcb9c636704441298518f400d4
https://doi.org/10.15593/2499-9873/2022.03.03
https://doi.org/10.15593/2499-9873/2022.03.03
Publikováno v:
Astronomy Reports. 66:648-668
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3bb65ec86db5318cd7c82f29a04bcdd8
https://doi.org/10.1134/s1063772922090025
https://doi.org/10.1134/s1063772922090025
Autor:
G. M. Rudnitskij, E. E. Lekht, N. T. Ashimbaeva, Krasnov, P. Colom, A. M. Tolmachev, M. I. Pashchenko
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:3285-3291
The aim of this work was to continue the monitoring of the H2O maser emission in IRAS 16293–2422 to detect superflares. We have been observing H2O maser emission at a wavelength of 1.35 cm towards the source IRAS 16293–2422 since 1999. The observ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::37ff6c2ccea9bfc3014df0e26b49667c
https://doi.org/10.1093/mnras/stab2287
https://doi.org/10.1093/mnras/stab2287
Publikováno v:
Astronomy Reports. 65:45-60
The monitoring results of the OH maser source in W75 N in the main line at 1665 MHz performed in 2007–2020 using the Nancay Radio Telescope (France) are presented. Generally, the maser in 2007–2009 is characterized by a high activity. During the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::26ec2666c97b1d6228912976e0f053aa
https://doi.org/10.1134/s1063772921010017
https://doi.org/10.1134/s1063772921010017
Autor:
E. E. Lekht, G. M. Rudnitskii, M. I. Pashchenko, N. T. Ashimbaeva, V. V. Krasnov, A. M. Tolmachev, P. Colom
Publikováno v:
Astronomy Reports. 64:839-854
We present the results of our observations of the star-forming region located in the Perseus arm and associated with the Sharpless nebula S231 in the lines of H2O at a wavelength of 1.35 cm and OH at a wavelength of 18 cm obtained with the Pushchino
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::441d18e56ba99abe5538cac1e58160d7
https://doi.org/10.1134/s1063772920110013
https://doi.org/10.1134/s1063772920110013
Autor:
Jiří Hejtmánek, Karel Knížek, Petr Levinský, Cestmir Drasar, M. I. Pashchenko, Tomáš Kmječ, Jiří Navrátil, Lenka Kubíčková
Publikováno v:
The Journal of Physical Chemistry C. 124:20773-20783
Our study targets some of the long-standing questions concerning the somewhat mysterious properties of chalcopyrite CuFeS2. We show that defect chemistry in connection with charge transfer within t...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1b2310a361c79f40223e72c72a06788c
https://doi.org/10.1021/acs.jpcc.0c06490
https://doi.org/10.1021/acs.jpcc.0c06490
Autor:
N. T. Ashimbaeva, P. Colom, E. E. Lekht, A. M. Tolmachev, G. M. Rudnitskii, M. I. Pashchenko, V. V. Krasnov
Publikováno v:
Astronomy Reports. 64:586-601
We present the observation results of the star forming region NGC 2071 in the 1.35-cm H2O line and 18-cm OH lines obtained with the 22-m radio telescope in Pushchino (Russia) and the large radio telescope in Nancay (France), respectively. The catalog
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::419dc88f93d13a33621881b7397a19a7
https://doi.org/10.1134/s1063772920080028
https://doi.org/10.1134/s1063772920080028
Autor:
Jiří Hejtmánek, Karel Knížek, Jiří Navrátil, Peter Baláž, Petr Levinský, Erika Dutková, M. I. Pashchenko, Philippe Masschelein
Publikováno v:
Acta Physica Polonica A. 137:904-907
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::52369a07813134f8f3cd7d9fcbb2c1a1
https://doi.org/10.12693/aphyspola.137.904
https://doi.org/10.12693/aphyspola.137.904
Autor:
N. T. Ashimbaeva, G. M. Rudnitskii, M. I. Pashchenko, A. M. Tolmachev, V. V. Krasnov, E. E. Lekht
Publikováno v:
Astronomy Reports. 64:15-22
The structure and evolution of powerful H2O maser flares in the source IRAS 18316–0602 are studied using the results of observations on the 22-m radio telescope of the Pushchino Radio Astronomy Observatory. The main origin of the last powerful, sho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d37e6e8cb7f4531588a2aaab174afd3b
https://doi.org/10.1134/s1063772920010011
https://doi.org/10.1134/s1063772920010011
Autor:
T. Zajarniuk, A. Szewczyk, P. Wiśniewski, M. U. Gutowska, R. Puzniak, H. Szymczak, I. Gudim, V. A. Bedarev, M. I. Pashchenko, P. Tomczak, W. Szuszkiewicz
Publikováno v:
Physical Review B. 105
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::04dfbe071bc061c0634e190405044978
https://doi.org/10.1103/physrevb.105.094418
https://doi.org/10.1103/physrevb.105.094418