|Authors||Richard de Grijs 1, Jessica T. Lee 2, M. Clemencia, Mora Herrera 3, Uta Fritze--v. Alvensleben 4, Peter Anders 4|
|Affiliation||1 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK, |
2 Department of Earth and Planetary Sciences, Harvard University, 20 Oxford Street, Cambridge, MA 02138, USA,
3 Departamento de Astronomía y Astrofísica, Facultad de Física, Pontifícia Universidad Católica de Chile, V. Vicuña Mackenna 4860 Macul, Santiago, Chile,
4 Universitätssternwarte, University of Göttingen, Geismarlandstr. 11, 37083 Göttingen, Germany
|Accepted by||New Astronomy|
In each interacting system we find some 40 bright young star clusters 20 < F606W (mag) < 25, with a characteristic mass of ~ 3 x 106 Mo), which are spatially coincident with blue regions of active star formation in their tidal tails and spiral arms. We estimate that the main events triggering the formation of these clusters occurred ~ (1.5-2.0) x 108 yr ago. We show that star cluster formation is a major mode of star formation in galaxy interactions, with > 35% of the active star formation in encounters occurring in star clusters. This is the first time that young star clusters have been detected along the tidal tails in interacting galaxies.
The tidal tail of the Tadpole system is dominated by blue star forming regions, which occupy some 60% of the total area covered by the tail and contribute ~ 70% of the total flux in the F475W filter (decreasing to ~ 40% in F814W). The remaining pixels in the tail have colours consistent with those of the main disk. The tidally triggered burst of star formation in the Mice is of similar strength in both interacting galaxies, but it has affected only relatively small, spatially coherent areas.