A dwarf irregular galaxy at the edge of the local group: Stellar populations and distance of IC5152

dc.contributor.authorZijlstra, AA
dc.contributor.authorMinniti, D
dc.date.accessioned2025-01-21T01:32:07Z
dc.date.available2025-01-21T01:32:07Z
dc.date.issued1999
dc.description.abstractWe have obtained V- and I-band photometry for about 700 stars in the field of the dwarf irregular galaxy IC 5152, previously considered a possible member of the Local Group. Deep VI color-magnitude diagrams are presented of the main body of this galaxy and of a nearby field. We infer a distance by comparison with the VI color-magnitude diagrams of similar galaxies and with theoretical isochrones. The distance modulus to IC 5152 is found to be m - M-o = 26.15 +/- 0.2, adopting E(V - I) = 0. This distance of D = 1.7 Mpc implies that IC 5152 is not a certain member of the Local Group. We also construct a deep optical luminosity function. By comparison with theoretical isochrones, we find a metallicity Z approximate to 0.002, which is lower than previous estimates. Using this metallicity and distance, IC 5152 now fits the metallicity-luminosity relation for dwarf galaxies. The youngest stars in the held studied have an age of similar to 10(7) Gyr, and there is a substantial population of stars with log t > 7.8-8 yr. The central region of IC 5152 is an active site of star formation, as found by comparing our optical photometry with Hubble Space Telescope ultraviolet images. Several candidate globular clusters are found, as well as a candidate for a potential nucleus.
dc.fuente.origenWOS
dc.identifier.issn0004-6256
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/97208
dc.identifier.wosidWOS:000080224500010
dc.issue.numero4
dc.language.isoen
dc.pagina.final1757
dc.pagina.inicio1743
dc.revistaAstronomical journal
dc.rightsacceso restringido
dc.subjectgalaxies : individual (IC 5152, IRAS 21594-51, ESO 237-27)
dc.subjectgalaxies : irregular
dc.subjectgalaxies : stellar content
dc.subjectgalaxy : formation
dc.subjectLocal Group
dc.titleA dwarf irregular galaxy at the edge of the local group: Stellar populations and distance of IC5152
dc.typeartículo
dc.volumen117
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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