Theory of the continuous spectrum of gaseous nebula of pure hydrogen
It has been studied the formation of the continuum of nebular hydrogen when ionization is due to radiation and to collisions. Two photon emission and continuous emissivity in the reaction of formation of H- have been included. The continuum results extremely sensitive to the relative amount of the t...
Guardado en:
| Autores principales: | Gerola, H., Panagia, N. |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1970
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/97840 |
| Aporte de: |
Ejemplares similares
-
The hydrogen line spectrum of gaseous nebulae
por: Gerola, H., et al.
Publicado: (1971) -
On the spectrum of a gaseous nebula of pure hydrogen, II
por: Gerola, H., et al. -
On the spectrum of a gaseous nebula of pure hydrogen, II
por: Gerola, H.
Publicado: (1970) -
On the spectrum of a gaseous nebula of pure hydrogen - III: The Balmer decrement
por: Gerola, H., et al. -
Collisional excitation in nebulae and symbiotic variables
por: Gerola, H., et al.
Publicado: (1970)