The paschen discontinuity in B stars

Autores
Ringuelet, Adela Emilia
Año de publicación
1969
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Measurements of the Paschen discontinuity in stars withT eff ≥104K leads to the conclusion that the D P/DB ratio increases with temperature faster than expected. The increase of D P/DB with (logg)−1 is also steep.
Les mesures de la discontinuité de Paschen dans les étoiles deT eff ≥104K nous montrent que le rapport D P/DB augmente avec la température plus rapidement que prevu. L'augment de D P/DB avec (logg)−1 est aussi remarquable.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Astronomía
Ciencias Astronómicas
Paschen discontinuity
Balmer discontinuity
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:10915/131085
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/131085
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling The paschen discontinuity in B starsRinguelet, Adela EmiliaAstronomíaCiencias AstronómicasPaschen discontinuityBalmer discontinuityMeasurements of the Paschen discontinuity in stars withT eff ≥104K leads to the conclusion that the D P/DB ratio increases with temperature faster than expected. The increase of D P/DB with (logg)−1 is also steep.Les mesures de la discontinuité de Paschen dans les étoiles deT eff ≥104K nous montrent que le rapport D P/DB augmente avec la température plus rapidement que prevu. L'augment de D P/DB avec (logg)−1 est aussi remarquable.Facultad de Ciencias Astronómicas y Geofísicas1969info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf459-468http://sedici.unlp.edu.ar/handle/10915/131085enginfo:eu-repo/semantics/altIdentifier/issn/0004-640xinfo:eu-repo/semantics/altIdentifier/issn/1572-946xinfo:eu-repo/semantics/altIdentifier/doi/10.1007/bf00652395info: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:UNLP2025-10-22T17:12:37Zoai:sedici.unlp.edu.ar:10915/131085Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:12:37.564SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv The paschen discontinuity in B stars
title The paschen discontinuity in B stars
spellingShingle The paschen discontinuity in B stars
Ringuelet, Adela Emilia
Astronomía
Ciencias Astronómicas
Paschen discontinuity
Balmer discontinuity
title_short The paschen discontinuity in B stars
title_full The paschen discontinuity in B stars
title_fullStr The paschen discontinuity in B stars
title_full_unstemmed The paschen discontinuity in B stars
title_sort The paschen discontinuity in B stars
dc.creator.none.fl_str_mv Ringuelet, Adela Emilia
author Ringuelet, Adela Emilia
author_facet Ringuelet, Adela Emilia
author_role author
dc.subject.none.fl_str_mv Astronomía
Ciencias Astronómicas
Paschen discontinuity
Balmer discontinuity
topic Astronomía
Ciencias Astronómicas
Paschen discontinuity
Balmer discontinuity
dc.description.none.fl_txt_mv Measurements of the Paschen discontinuity in stars withT eff ≥104K leads to the conclusion that the D P/DB ratio increases with temperature faster than expected. The increase of D P/DB with (logg)−1 is also steep.
Les mesures de la discontinuité de Paschen dans les étoiles deT eff ≥104K nous montrent que le rapport D P/DB augmente avec la température plus rapidement que prevu. L'augment de D P/DB avec (logg)−1 est aussi remarquable.
Facultad de Ciencias Astronómicas y Geofísicas
description Measurements of the Paschen discontinuity in stars withT eff ≥104K leads to the conclusion that the D P/DB ratio increases with temperature faster than expected. The increase of D P/DB with (logg)−1 is also steep.
publishDate 1969
dc.date.none.fl_str_mv 1969
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/10915/131085
url http://sedici.unlp.edu.ar/handle/10915/131085
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0004-640x
info:eu-repo/semantics/altIdentifier/issn/1572-946x
info:eu-repo/semantics/altIdentifier/doi/10.1007/bf00652395
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
459-468
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
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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