Отрывок: Obviously, to follow all these transformations, one needs to construct an evolutionary model. which would account for various changes in the dust size distribution, charge state, bond structure, etc. [12]. The studies at Lebedev Physical Institute were supported by the Ministry of Science and Higher Education of the Russian Federation by the grant No. 075-15-2021-597. References 1. A.P. Jones et al., Astron. and Astrophys. 2013...
Полная запись метаданных
Поле DC | Значение | Язык |
---|---|---|
dc.contributor.author | Wiebe D. | ru |
dc.coverage.spatial | межзвездная среда | ru |
dc.coverage.spatial | межзвездная пыль | ru |
dc.coverage.spatial | полициклические ароматические углеводороды | ru |
dc.coverage.spatial | углеродсодержащие частицы | ru |
dc.coverage.spatial | ультрафиолетовое излучение | ru |
dc.coverage.spatial | ароматические соединения | ru |
dc.coverage.spatial | ultraviolet radiation | ru |
dc.coverage.spatial | interstellar dust | ru |
dc.coverage.spatial | polycyclic aromatic hydrocarbons | ru |
dc.coverage.spatial | interstellar medium | ru |
dc.coverage.spatial | aromatic compounds | ru |
dc.coverage.spatial | carbonbearing particles | ru |
dc.creator | Wiebe D. | ru |
dc.date.accessioned | 2022-10-06 14:29:35 | - |
dc.date.available | 2022-10-06 14:29:35 | - |
dc.date.issued | 2022 | ru |
dc.identifier | RU\НТБ СГАУ\487893 | ru |
dc.identifier.citation | Wiebe, D. Carbon Dust Life Cycle in the Universe / D. Wiebe // International Conference on Physics and Chemistry of Combustion and in Extreme Environments (Samara, Russia, 12-16 July 2022) / V. N. Azyazov, A. M. Mayorova. - Samara : Publishing OOO “Insoma-Press”, 2022. - P. 28. | ru |
dc.identifier.uri | http://repo.ssau.ru/handle/International-Conference/Carbon-Dust-Life-Cycle-in-the-Universe-98896 | - |
dc.language.iso | eng | ru |
dc.source | International Conference on Physics and Chemistry of Combustion and in Extreme Environments (Samara, Russia, 12-16 July 2022) | ru |
dc.title | Carbon Dust Life Cycle in the Universe | ru |
dc.type | Text | ru |
dc.textpart | Obviously, to follow all these transformations, one needs to construct an evolutionary model. which would account for various changes in the dust size distribution, charge state, bond structure, etc. [12]. The studies at Lebedev Physical Institute were supported by the Ministry of Science and Higher Education of the Russian Federation by the grant No. 075-15-2021-597. References 1. A.P. Jones et al., Astron. and Astrophys. 2013... | - |
Располагается в коллекциях: | International Conference on Combustion Physics and Chemistry |
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978-5-4317-0481-9_2022-28.pdf | 452.67 kB | Adobe PDF | Просмотреть/Открыть |
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