Gas Flow and Star Formation in the `Antennae' Galaxies NGC 4038/9

Astronomy and Astrophysics – Astrophysics

Scientific paper

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To appear in proceedings of Gas and Galaxy Evolution, (VLA 20th Anniversary Conference), ASP Conf. Series, ed. J. Hibbard, M.

Scientific paper

The prominent interacting galaxy pair NGC 4038/9 contains many active star-forming regions and is continuously forming new star clusters. We present a self-consistent n-body model for this system which includes an SPH gas component. The model qualitatively explains the apparent concentration of gas in the so-called overlap region between the two nuclei as a bridge of gas connecting the two galaxies. Projected on the sky, the bridge appears as a dense spot of gas. We discuss some implications for the evolution of Ultra-luminous infrared galaxies.

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