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dc.date.accessioned | 2022-11-08T12:56:57Z | |
dc.date.available | 2022-11-08T12:56:57Z | |
dc.date.issued | 1992 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/145303 | |
dc.description.abstract | We present integrated Washington photometry (C,M,T₁) of globular clusters in the held of NGC 1399. Conflicting evidence on the presence of a (B-V) color gradient as a function of galactocentric distance has been reported for this cluster system. Here we investigate the existence of this gradient using the (C-T₁) index, which is twice as metallicity sensitive as (B-V). | en |
dc.language | es | es |
dc.subject | Galaxia | es |
dc.subject | ngc 1399 | es |
dc.title | Metallicity gradient in the globular cluster system around NGC 1399 | en |
dc.type | Articulo | es |
sedici.identifier.issn | 1669-9521 | es |
sedici.creator.person | Ostrov, Pablo Gabriel | es |
sedici.creator.person | Geisler, D. | es |
sedici.creator.person | Forte, 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. 37 | 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) |