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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