Search for evidence of radiative equilibrium departures in extended atmospheres

Autores
Venero, Roberto Oscar José; Cidale, Lydia Sonia; Ringuelet, Adela Emilia
Año de publicación
2000
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Through the analysis of line profiles of atoms in different ionization stages, we study the source function behavior of those elements that allow us to outline temperature structures in moving extended atmospheres. The radiative transfer equation is solved in the comoving frame and NLTE for multilevel atoms.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Física
Line profiles of atoms
Ionization
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/146092

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spelling Search for evidence of radiative equilibrium departures in extended atmospheresVenero, Roberto Oscar JoséCidale, Lydia SoniaRinguelet, Adela EmiliaFísicaLine profiles of atomsIonizationThrough the analysis of line profiles of atoms in different ionization stages, we study the source function behavior of those elements that allow us to outline temperature structures in moving extended atmospheres. The radiative transfer equation is solved in the comoving frame and NLTE for multilevel atoms.Facultad de Ciencias Astronómicas y Geofísicas2000info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf607-610http://sedici.unlp.edu.ar/handle/10915/146092enginfo:eu-repo/semantics/altIdentifier/issn/0252-9211info:eu-repo/semantics/altIdentifier/doi/10.1017/s0252921100056621info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:32:27Zoai:sedici.unlp.edu.ar:10915/146092Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:32:27.994SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Search for evidence of radiative equilibrium departures in extended atmospheres
title Search for evidence of radiative equilibrium departures in extended atmospheres
spellingShingle Search for evidence of radiative equilibrium departures in extended atmospheres
Venero, Roberto Oscar José
Física
Line profiles of atoms
Ionization
title_short Search for evidence of radiative equilibrium departures in extended atmospheres
title_full Search for evidence of radiative equilibrium departures in extended atmospheres
title_fullStr Search for evidence of radiative equilibrium departures in extended atmospheres
title_full_unstemmed Search for evidence of radiative equilibrium departures in extended atmospheres
title_sort Search for evidence of radiative equilibrium departures in extended atmospheres
dc.creator.none.fl_str_mv Venero, Roberto Oscar José
Cidale, Lydia Sonia
Ringuelet, Adela Emilia
author Venero, Roberto Oscar José
author_facet Venero, Roberto Oscar José
Cidale, Lydia Sonia
Ringuelet, Adela Emilia
author_role author
author2 Cidale, Lydia Sonia
Ringuelet, Adela Emilia
author2_role author
author
dc.subject.none.fl_str_mv Física
Line profiles of atoms
Ionization
topic Física
Line profiles of atoms
Ionization
dc.description.none.fl_txt_mv Through the analysis of line profiles of atoms in different ionization stages, we study the source function behavior of those elements that allow us to outline temperature structures in moving extended atmospheres. The radiative transfer equation is solved in the comoving frame and NLTE for multilevel atoms.
Facultad de Ciencias Astronómicas y Geofísicas
description Through the analysis of line profiles of atoms in different ionization stages, we study the source function behavior of those elements that allow us to outline temperature structures in moving extended atmospheres. The radiative transfer equation is solved in the comoving frame and NLTE for multilevel atoms.
publishDate 2000
dc.date.none.fl_str_mv 2000
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/146092
url http://sedici.unlp.edu.ar/handle/10915/146092
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0252-9211
info:eu-repo/semantics/altIdentifier/doi/10.1017/s0252921100056621
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
607-610
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
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instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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