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dc.date.accessioned 2022-09-13T14:12:42Z
dc.date.available 2022-09-13T14:12:42Z
dc.date.issued 1988
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/141993
dc.description.abstract The continuum radiations at 1420 MHz, coming from the Gum nebula region centered around the point of galactic coordinates 1 = 263° , b = +7° and detected with the radiotelescope of the IAR, are compared with that registered at 408 MHz by Haslam et al. Contributions coming from the galactic and extragalactic backgrounds, and the thermal and synchrotron components for the nebula, are discriminated. For the latter, theoretical results are presented which allow for the determination of the spectral index corresponding to the energetic spectrum of the relativistic electrons. en
dc.language es es
dc.subject Galaxia es
dc.title Radio emission coming from a region of the gum nebulae en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Reynoso, E. es
sedici.creator.person Colomb, Fernando Raúl es
sedici.creator.person Piacentini, R.D. es
sedici.creator.person Testori, Juan Carlos es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion 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. 34 es
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/ es
dc.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) es


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