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
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/131085
Ver los metadatos del registro completo
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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 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/131085 |
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http://sedici.unlp.edu.ar/handle/10915/131085 |
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eng |
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eng |
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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) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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