Wide Field Observations of the Ursa Minor dSph galaxy

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dc.creatorMartinez-Delgado, D.
dc.creatorAparicio, A.
dc.date1999-04-28
dc.date.accessioned2026-07-07T02:31:25Z
dc.date.available2026-07-07T02:31:25Z
dc.descriptionUrsa Minor (UMi) is one of the closest satellites of the Milky Way (d=69 kpc). It is possibly a disrupted dSph interacting with the external Galactic halo. This makes its study quite necessary in the forementioned context. In this paper we present preliminary results of a wide field photometry survey of UMi and discuss the presence of an intermediate-age population and tidal tails in it.
dc.description4 pages, 5 figures, to appear in the IAU Symp.192 Proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/9904385
dc.identifierhttp://arxiv.org/abs/astro-ph/9904385
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14147
dc.subjectAstrophysics
dc.titleWide Field Observations of the Ursa Minor dSph galaxy
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