On the spectrum of a gaseous nebula of pure hydrogen - III: The Balmer decrement
The Balmer decrement was calculated for a homogeneous, spherical, pure hydrogen nebula, ionised and excited both by radiative and collisional processes. Reabsorption in the Balmer series from sublevels 2 s and 2 p was taken into account. Calculations were carried out for electron temperatures of 104...
| Autor principal: | Salem, M. |
|---|---|
| Publicado: |
1971
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004640X_v10_n3_p383_Gerola http://hdl.handle.net/20.500.12110/paper_0004640X_v10_n3_p383_Gerola |
| Aporte de: |
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