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Non-LTE effects for Na I lines in X-ray illuminated stellar atmospheresThe formation of Na I lines in X-ray illuminated atmospheres is investigated by abandoning
Interaction of N-vortex structures in a continuum, including atmosphere, hydrosphere and plasma© 2017 COSPAR The results of analysis and numerical simulation of evolution and interaction
Interaction of N-vortex structures in a continuum, including atmosphere, hydrosphere and plasma© 2017 COSPAR The results of analysis and numerical simulation of evolution and interaction
Non-LTE effects for Na I lines in X-ray illuminated stellar atmospheresThe formation of Na I lines in X-ray illuminated atmospheres is investigated by abandoning
Effect of atomic parameters on determination of aluminium abundance in atmospheres of late-type stars on the inferred aluminium abundance in stellar atmospheres. We match the theoretical and observed line profiles
Investigation of Cyg OB2 #11(O5 Ifc) by modelling its atmosphere-resolution spectra. In this paper we present results of the modelling of the stellar atmosphere of Cyg OB2 #11
Escape of rock-forming volatile elements and noble gases from planetary embryos-lived radioactive elements. During their solidification after the dissipation of the disk a steam atmosphere
Effect of atomic parameters on determination of aluminium abundance in atmospheres of late-type stars on the inferred aluminium abundance in stellar atmospheres. We match the theoretical and observed line profiles
Investigation of Cyg OB2 #11(O5 Ifc) by modelling its atmosphere-resolution spectra. In this paper we present results of the modelling of the stellar atmosphere of Cyg OB2 #11
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