The Distance to Hydra and Centaurus From Surface Brightness Fluctuations: Consequences for the Great Attractor Model

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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.issued2005
dc.identifier.issn0004-6361
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/19118
dc.language.isoen
dc.relation.isformatofAstronomy & Astrophysics. Vol. 438, no. 1 (2005), p. [103]-119
dc.revistaAstronomy & Astrophysicses_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherGalaxias - Cúmuloses_ES
dc.subject.otherGalaxias - Medicioneses_ES
dc.subject.otherFotometría astronómicaes_ES
dc.titleThe Distance to Hydra and Centaurus From Surface Brightness Fluctuations: Consequences for the Great Attractor Modeles_ES
dc.typeartículo
sipa.codpersvinculados55248
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