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dc.date.accessioned 2022-09-26T12:46:32Z
dc.date.available 2022-09-26T12:46:32Z
dc.date.issued 1990
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/142704
dc.description.abstract The Gum Nebula, with a diameter of 36" and surrounded by Hα filaments, is one of the more extended features on the sky. Within that region several interesting objects as Vela, Puppis and RCW 38, are found. For this reason we decided to map this extended region with high sensitivity at the frequency of 1435 MHz. A reduction method was developed that allowed to calibrate absolutely the observations and to obtain the Spectral Index (Tb=f⁻ᵇ), comparing our observations with those obtained by Haslam et al. (1982). en
dc.language es es
dc.subject Galaxia es
dc.subject gum nebula es
dc.title Radio continuum observations of the Gum Nebula en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Testori, Juan Carlos es
sedici.creator.person Colomb, Fernando Raúl 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. 36 es
dc.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)


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