The radio spectrum of the galaxy

Autores
Burke, B.P.
Año de publicación
1968
Idioma
español castellano
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The progress of human knowledge often seems to come in sudden bursts of activity, with resting periods in between, when the new concepts are exploited, fitted into existing pictures of the physical world, or the pictures of the world modified to fit the new insights. In astrophysics, radio spectroscopy may well be in the midst of such an active phase. Two decades have passed since van de Hulst suggested, in 1904, that the ground state hyper-fine transition in Hydrogen, the celebrated 21-cm line, should be an exceptionally useful tool in studying the galaxy.
Asociación Argentina de Astronomía
Materia
Astronomía
Galaxias
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:10915/93069
Acceder
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spelling The radio spectrum of the galaxyBurke, B.P.AstronomíaGalaxiasThe progress of human knowledge often seems to come in sudden bursts of activity, with resting periods in between, when the new concepts are exploited, fitted into existing pictures of the physical world, or the pictures of the world modified to fit the new insights. In astrophysics, radio spectroscopy may well be in the midst of such an active phase. Two decades have passed since van de Hulst suggested, in 1904, that the ground state hyper-fine transition in Hydrogen, the celebrated 21-cm line, should be an exceptionally useful tool in studying the galaxy.Asociación Argentina de Astronomía1968info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/93069spainfo:eu-repo/semantics/altIdentifier/issn/1669-9521info: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:UNLP2025-10-22T17:00:11Zoai:sedici.unlp.edu.ar:10915/93069Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:00:11.717SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv The radio spectrum of the galaxy
title The radio spectrum of the galaxy
spellingShingle The radio spectrum of the galaxy
Burke, B.P.
Astronomía
Galaxias
title_short The radio spectrum of the galaxy
title_full The radio spectrum of the galaxy
title_fullStr The radio spectrum of the galaxy
title_full_unstemmed The radio spectrum of the galaxy
title_sort The radio spectrum of the galaxy
dc.creator.none.fl_str_mv Burke, B.P.
author Burke, B.P.
author_facet Burke, B.P.
author_role author
dc.subject.none.fl_str_mv Astronomía
Galaxias
topic Astronomía
Galaxias
dc.description.none.fl_txt_mv The progress of human knowledge often seems to come in sudden bursts of activity, with resting periods in between, when the new concepts are exploited, fitted into existing pictures of the physical world, or the pictures of the world modified to fit the new insights. In astrophysics, radio spectroscopy may well be in the midst of such an active phase. Two decades have passed since van de Hulst suggested, in 1904, that the ground state hyper-fine transition in Hydrogen, the celebrated 21-cm line, should be an exceptionally useful tool in studying the galaxy.
Asociación Argentina de Astronomía
description The progress of human knowledge often seems to come in sudden bursts of activity, with resting periods in between, when the new concepts are exploited, fitted into existing pictures of the physical world, or the pictures of the world modified to fit the new insights. In astrophysics, radio spectroscopy may well be in the midst of such an active phase. Two decades have passed since van de Hulst suggested, in 1904, that the ground state hyper-fine transition in Hydrogen, the celebrated 21-cm line, should be an exceptionally useful tool in studying the galaxy.
publishDate 1968
dc.date.none.fl_str_mv 1968
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info:eu-repo/semantics/publishedVersion
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status_str publishedVersion
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dc.language.none.fl_str_mv spa
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dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/1669-9521
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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
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rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
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