Dusty plasma influence on some atmospheric layers of very low-mass stars and brown dwarfs
|1Martysh, EV, 2Danilova, VV |
1Space Research Institute of the National Academy of Sciences of Ukraine and the National Space Agency of Ukraine, Kyiv, Ukraine
2Taras Shevchenko National University of Kyiv, Kyiv, Ukraine
|Kosm. nauka tehnol. 2007, 13 ;(1):079-082|
|Язык публикации: Ukrainian|
We consider the possibility to use the dusty magnetized plasma as a model medium for some atmospheric layers of VLM-stars and brown dwarfs. The influence of magnetic field on the thermodynamic parameters of the system is analyzed. A new mechanism of the radiation of the objects under investigation in the long-wave portion of RF range is proposed. Evaluation of the phenomena mentioned is performed.
|Ключевые слова: magnetic field, mechanism of the radiation, thermodynamic parameters|
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