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dc.date.accessioned 2022-02-16T12:08:18Z
dc.date.available 2022-02-16T12:08:18Z
dc.date.issued 1987
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/131134
dc.description.abstract Results from photoelectric photometry in molecular bands of comet Hally carried out at Bosque Alegre are presented. The largest emissions measured are those of molecules of C₂, CN and C₃, respectively. NO detectable contribution exists from the CO⁺ ion. Decreases in the fluxes, observed with a periodicity P=6ᵈ.10 + 0ᵈ.02 coincide with desconnection events detected at Bosque Alegre and other observatories. If they correspond to the frequency of passage of magnetic solar sectors by the comet, a solar "sinodic" rotation period P_c= 24ᵈ.4 + 0ᵈ.8, with respect to the comet, is deduced, in every good agreement with the mean value of the apparetn solar rotation with respect to the comet. en
dc.language es es
dc.subject Galaxias es
dc.title Estudio fotométrico de emisiones moleculares del cometa Halley en la etapa post-perihelio es
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Sisteró, Roberto Félix es
sedici.creator.person Clariá Olmedo, Juan José es
sedici.creator.person Lapasset, Emilio 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. 32 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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