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The Taffy galaxy pair : optical and radio characterization of an interacting system

J. Saponara ... [et al.].

Serie: Trabajos publicados del IAR ; no. 1704

Resumen: The Taffy galaxy pair UGC 12915/4 constitutes an excellent example of an ongoing major gas-rich merger. Evidence suggests that the two galaxies experienced a head-on collision 25-30 Myr ago that raised an atomic and molecular gas bridge connecting both galaxies. This system has been poorly studied in the optical and near-infrared. Therefore, we observe the whole Taffy system with Gemini-North in g', r', i', z', Hα, and HαC bands. We aim to characterise the optical counterparts of several Ultra Luminous X-ray sources (ULXs), detect star clusters, extragalactic star-forming regions, and identify low-mass galaxies of tidal origin. We expect that this additional information will help to better understand the physical processes involved in galaxy interactions

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Boletín de la Asociación Argentina de Astronomía ISSN 0571-3285 — Vol. 63, (2022), p. 250-252
 
Registro 001920 · Modificado: 11/10/2022

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