Potential of the Surface Brightness Fluctuations Method to Measure Distances to Dwarf Elliptical Galaxies in Nearby Clusters

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dc.contributor.authorMieske, S.
dc.contributor.authorInfante Lira, Leopoldo
dc.date.accessioned2017-04-11T20:51:39Z
dc.date.available2017-04-11T20:51:39Z
dc.date.issued2003
dc.identifier.doi10.1051/0004-6361:20030331
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361:20030331
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/19117
dc.language.isoen
dc.relation.isformatofAstronomy & Astrophysics. Vol. 403, no. 1 (2003), p. [43]-53
dc.revistaAstronomy & Astrophysicses_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherGalaxias elípticases_ES
dc.subject.otherGalaxias enanases_ES
dc.subject.otherCúmulos de Galaxiases_ES
dc.subject.otherAstronomía - Observacioneses_ES
dc.titlePotential of the Surface Brightness Fluctuations Method to Measure Distances to Dwarf Elliptical Galaxies in Nearby Clusterses_ES
dc.typeartículo
sipa.codpersvinculados55248
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