Zobrazeno 1 - 6
of 6
pro vyhledávání: '"M E Kalyashova"'
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ce9a4c700fe3bcf633a15d28b4fe947c
https://doi.org/10.3103/s1062873823702313
https://doi.org/10.3103/s1062873823702313
Young massive star clusters inhabit regions of star formation and play an essential role in the galactic evolution. They are sources of both thermal and non-thermal radiation, and they are effective cosmic ray accelerators. We present the 3D magnetoh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2e7dabf516c95cc4495e5ad2b962df1
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 85:357-359
An excess of 22Ne/20Ne in the isotopic composition of cosmic rays was discovered more than 40 years ago. Isotopic ratio 22Ne/20Ne measured in cosmic rays is more than five times higher than in the solar wind. It was proposed that processes in Wolf–
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5ce84031f93771bd1e5310e3268821f4
https://doi.org/10.3103/s1062873821040146
https://doi.org/10.3103/s1062873821040146
Autor:
M E Kalyashova, A M Bykov
Publikováno v:
Journal of Physics: Conference Series. 2103:012008
22Ne/20Ne isotopic ratio is found to be about 5 times higher in Galactic cosmic rays (GCRs) than in the solar wind. In this paper we develop the hypothesis that the 22Ne overabundance in CRs is generated in compact massive star clusters which contain
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b4971176a6e36445d49a685d0ebfdaf9
https://doi.org/10.1088/1742-6596/2103/1/012008
https://doi.org/10.1088/1742-6596/2103/1/012008
Publikováno v:
Journal of Physics: Conference Series. 1038:012017
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e7b372c36619c0054971853137cb44fb
https://doi.org/10.1088/1742-6596/1038/1/012017
https://doi.org/10.1088/1742-6596/1038/1/012017
Publikováno v:
Journal of Physics: Conference Series; 2018, Vol. 1038 Issue 1, p1-1, 1p