Abstract
We present here preliminary results of our wide-field study of NGC 3109: a low luminosity galaxy in the outskirts of the Local Group. Its edge-on orientation (which simplifies the study of a possible halo) and the possibility that it could, in fact, be a small spiral (the smallest in the Local Group) makes its deep analysis of major relevance to understand the properties of dwarf galaxies and the transition from dwarf irregulars to spirals.
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© 2002 Springer Science+Business Media Dordrecht
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Hidalgo, S.L., Aparicio, A. (2002). NGC 3109: Halo/Disk Structures in Faint Galaxies. In: Sauvage, M., Stazińska, G., Schaerer, D. (eds) The Evolution of Galaxies. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3311-3_17
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DOI: https://doi.org/10.1007/978-94-017-3311-3_17
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-6020-4
Online ISBN: 978-94-017-3311-3
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