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Chromospheric NLTE-Radiative-Transfer Modeling of dMe Stars
Published online by Cambridge University Press: 27 September 2017
Abstract
The formation of the Lyman and Balmer lines of Hydrogen at densities typical in dMe stars is shown to be very dependent on the atomic model used viz. the number of levels and line transitions. The effect of increasing the number of levels and line transitions on the line fluxes and ionization fraction is also discussed.
- Type
- Session III: Theory
- Information
- International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 361 - 364
- Copyright
- Copyright © Kluwer 1989