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A&A 399, 489-496 (2003)
DOI: 10.1051/0004-6361:20021810
Globular cluster candidates within the Fornax Cluster: Intracluster globulars?
L. P. Bassino1, 2, S. A. Cellone1, J. C. Forte1, 2 and B. Dirsch31 Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque S/N, 1900-La Plata, Argentina
2 Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Argentina
3 Universidad de Concepción, Departamento de Física, Casilla 160-C, Concepción, Chile
(Received 24 July 2002 / Accepted 22 November 2002)
Abstract
We present the results of a search for globular clusters in
the surroundings of 15 low surface brightness dwarf galaxies belonging
to the Fornax Cluster, which was carried out on CCD images obtained with
the
C and
T1 filters of the Washington photometric system.
The globular cluster candidates show an extended and probably
bimodal
(C-T1) color
distribution, which is inconsistent with the presence of a single
population of metal-poor clusters detected in several dwarf galaxies.
The surface number density of these candidates shows no
concentration towards the respective dwarf galaxies, in whose outskirts
they have been identified.
On the contrary, if we split the candidates in two groups according
to their projected distances to the center of the Fornax Cluster, those
located closer to the center show a higher projected density
than those located farther from it. These results suggest that
the potential globular clusters might not be bound to the dwarf
galaxies. Alternatively, these globulars could form part of the very
peripheral regions of
NGC 1399
(the central galaxy of the Fornax
Cluster) or even belong to the intracluster medium.
Key words: Galaxy: globular clusters: general -- galaxies: star clusters -- galaxies: dwarf -- galaxies: clusters: individual Fornax
Offprint request: L. P. Bassino, lbassino@fcaglp.fcaglp.unlp.edu.ar
© ESO 2003
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