The hydrogen line spectrum of gaseous nebulae

The relative intensities of the hydrogen emission lines of homogeneous gaseous nebulae, ionized and excited by riative and collisional processes, have been calculated. The results define allowed and forbidden regions in the Balmer colour-colour plot different from those obtained assuming purely radi...

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Detalles Bibliográficos
Autores principales: Gerola, H., Salem, M., Panagia, N.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1971
Materias:
Astronomía
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/98026
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-98026
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxias
spellingShingle Astronomía
Galaxias
Gerola, H.
Salem, M.
Panagia, N.
The hydrogen line spectrum of gaseous nebulae
topic_facet Astronomía
Galaxias
description The relative intensities of the hydrogen emission lines of homogeneous gaseous nebulae, ionized and excited by riative and collisional processes, have been calculated. The results define allowed and forbidden regions in the Balmer colour-colour plot different from those obtained assuming purely radiative or purely collisional excitation and ionization. A brief comparison with observational data is carried out.
format Articulo
Comunicacion
author Gerola, H.
Salem, M.
Panagia, N.
author_facet Gerola, H.
Salem, M.
Panagia, N.
author_sort Gerola, H.
title The hydrogen line spectrum of gaseous nebulae
title_short The hydrogen line spectrum of gaseous nebulae
title_full The hydrogen line spectrum of gaseous nebulae
title_fullStr The hydrogen line spectrum of gaseous nebulae
title_full_unstemmed The hydrogen line spectrum of gaseous nebulae
title_sort hydrogen line spectrum of gaseous nebulae
publishDate 1971
url http://sedici.unlp.edu.ar/handle/10915/98026
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