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dc.date.accessioned | 2022-09-22T15:09:03Z | |
dc.date.available | 2022-09-22T15:09:03Z | |
dc.date.issued | 1988 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/142578 | |
dc.description.abstract | The ionized gas in NGC 1313 was studied by spectro-photometric means. The radial behaviour of the I(Hα)/I(6584), I(6717)/I(6731), N(NII)/N(NHII) and N(NII)/N(SII) ratios and the deduced electron densities are discussed. The abundance ratios N(N)/N(H) and N(N)/N(S) for the nucleus and two emission regions were also derived and compared with the previous data. | en |
dc.language | es | es |
dc.subject | Galaxia | es |
dc.title | Some physical considerations about NGC 1313 | en |
dc.type | Articulo | es |
sedici.identifier.issn | 1669-9521 | es |
sedici.creator.person | Agüero, Estela Laura | 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 |