Zobrazeno 1 - 10
of 27
pro vyhledávání: '"S. I. Neizvestny"'
Publikováno v:
Открытое образование (Москва), Vol 27, Iss 5, Pp 45-56 (2023)
Relevance of the study. Any industrial revolution, any global innovation faces resistance caused by the fundamental properties of the human psyche – a wary attitude to change, fear of introducing innovations, distrust of future uncertainty. The mod
Externí odkaz:
https://doaj.org/article/513f012ef52742dc93de1059b442107f
Autor:
K. K. Kuchmezov, S. I. Neizvestny
Publikováno v:
Открытое образование (Москва), Vol 26, Iss 5, Pp 51-60 (2022)
The purpose of this study was to describe new approaches to the practical reaction of the educational process of training business informatics specialists to the modern challenges of digitalization of society in the field of formation of emotional in
Externí odkaz:
https://doaj.org/article/e0a29ccad536414397435c0030008ae7
Autor:
V. I. Marshev, S. I. Neizvestny
Publikováno v:
Управленческие науки, Vol 12, Iss 1, Pp 79-95 (2022)
The paper compares the state and solutions to the problems of forming and assessing the competencies of graduates of the educational system in the field of management in Russia in 19th century with the conditions of the digital society of modern post
Externí odkaz:
https://doaj.org/article/af87a06001d14210a8bcdaa4fef11f69
Autor:
H. H. Kuchmezov, S. I. Neizvestny
Publikováno v:
Открытое образование (Москва), Vol 26, Iss 2, Pp 25-36 (2022)
The purpose of this study is to analyze existing approaches to managing a portfolio of projects and programs, their further development and generalization, the creation of systems focused on creating the competence of specialists in the field of mana
Externí odkaz:
https://doaj.org/article/567e5514ee0c49ba9ea06c74b9ea9623
Publikováno v:
Astrophysics. 53:154-162
By observations with the 1.5m telescope at San Pedro Martir (OAN, UNAM, Mexico) the BVR magnitudes are determined for 66 member galaxies in Shakhbazian Compact Galaxy Groups ShCG 40, ShCG 176, ShCG 270, ShCG 278, ShCG 310, and ShCG 342. Three other g
Autor:
V. H. Chavushyan, S. I. Neizvestny, J. P. Torres-Papaqui, Gaghik H. Tovmassian, Hrant M. Tovmassian, S. G. Navarro, H. Tiersch
Publikováno v:
Astronomy Reports. 50:861-873
We continue the presentation of the results of detailed spectroscopic and photometric study of Shakhbazian compact galaxy groups. They belong to the interesting class of compact groups. Because of their large number (the catalogue contains 377 entrie
Autor:
V. H. Chavushyan, H. Tiersch, S. G. Navarro, Gaghik H. Tovmassian, J. P. Torres-Papaqui, Hrant M. Tovmassian, S. I. Neizvestny
Publikováno v:
Astronomy & Astrophysics. 439:973-979
We present the results of a detailed spectroscopic and photometric study of four Shakhbazian compact groups: ShCG 8, ShCG 14, ShCG 19, and ShCG 22. We determined the redshifts of member galaxies and radial velocity dispersions of groups. We also stud
Autor:
S. I. Neizvestny, J. P. Torres-Papaqui, Hrant M. Tovmassian, Gaghik H. Tovmassian, A. G. Pramskij, H. Tiersch
Publikováno v:
Astronomische Nachrichten. 326:362-369
In the course of investigation of Shakhbazian compact groups we studied the group ShCG 191 which has been identified also as the Abell cluster A1097. By its richness it may be classified as a rich compact group or a poor cluster. We determined redshi
Autor:
Gaghik H. Tovmassian, V. H. Chavushyan, H. Tiersch, Hrant M. Tovmassian, S. I. Neizvestny, S. G. Navarro
Publikováno v:
Astronomy & Astrophysics. 415:803-811
In 1995 we commenced a detailed spectral and photometric study of Shakhbazian compact groups. In this paper the results on groups ShCG 181, ShCG 344, ShCG 361, and ShCG 362 are presented. The redshifts of member galaxies in groups and the radial velo
Autor:
Hrant M. Tovmassian, A. S. Amirkhanian, H. T. MacGillivray, D. Stoll, S. I. Neizvestny, Hans Böhringer, H. Tiersch
Publikováno v:
Astronomy & Astrophysics. 392:33-52
Shakhbazian compact galaxy groups belong to the interesting class of compact groups. Because of their large number (the catalogue contains 377 entries) we are able to study the groups in dierent stages of evolution. Here we give the results of detail