Lyman alfa and excitation mechanism
Lyman alfa of hydrogen results to be the best indicator of the excitation mechanism operating in gaseous nebula. Also the interstellar absorption by gas and dust has been included. Recent observations with space probes may imply that also for interstellar gas collisional excitations is important.
Guardado en:
| Autores principales: | Gerola, H., Fulchignoni, M.M., Panagia, N. |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1970
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/98019 |
| Aporte de: |
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