Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2020-04-08T12:03:22Z
dc.date.available 2020-04-08T12:03:22Z
dc.date.issued 1968
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/93069
dc.description.abstract 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. en
dc.language es es
dc.subject Galaxias es
dc.title The radio spectrum of the galaxy en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Burke, B.P. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no.11 es


Descargar archivos

Thumbnail
Documento Completo
Descargar archivo (208.8Kb) - PDF

Este ítem aparece en la(s) siguiente(s) colección(ones)

Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)