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Are magnetically-powered phenomena on brown dwarfs similar to or very different from M dwarfs? PowerPoint PPT Presentation
Are magnetically-powered phenomena on brown dwarfs similar to or very different from M dwarfs? - ... nonLTE radiative/convective equilibrium models for M, L, T dwarfs ... VB 10 ... As Teff decreases the atmospheres become far less ionized and poor ...
... nonLTE radiative/convective equilibrium models for M, L, T dwarfs ... VB 10 ... As Teff decreases the atmospheres become far less ionized and poor ...
| PowerPoint PPT presentation | free to download
University of Illinois, UrbanaChampaign, USA PowerPoint PPT Presentation
University of Illinois, UrbanaChampaign, USA - University of Illinois, Urbana-Champaign, USA. PMOD/WRC, Switzerland. NASA/Goddard Space Flight Center, ... Photolysis rates for Ly- , Schumann-Runge continuum ...
University of Illinois, Urbana-Champaign, USA. PMOD/WRC, Switzerland. NASA/Goddard Space Flight Center, ... Photolysis rates for Ly- , Schumann-Runge continuum ...
| PowerPoint PPT presentation | free to view
The nonLTE Rate Equations PowerPoint PPT Presentation
The nonLTE Rate Equations - Element 1: NLTE-levels: ion1: 6, ion2: 4, ion3: 1. Element 2: NLTE-levels: ion1: 3, ion2: 5, ion3: 1. Element 3: NLTE-levels: ion1: 5, ion2: 1, hydrogen ...
Element 1: NLTE-levels: ion1: 6, ion2: 4, ion3: 1. Element 2: NLTE-levels: ion1: 3, ion2: 5, ion3: 1. Element 3: NLTE-levels: ion1: 5, ion2: 1, hydrogen ...
| PowerPoint PPT presentation | free to view


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