WFPC2 Observations of the Nuclear Starburst in NGC 253

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We present UVRI and Hα images of the nuclear starburst in NGC 253, a barred spiral galaxy located at a distance of only 3 Mpc. We resolve the nuclear region into many star-forming complexes, most of which are themselves resolved for the first time and have typical diameters of up to about 5 pc. We also resolve the brightest stars in the circumnuclear region. The Hα emission lies in a fan to the SE of the nucleus, and both it and dust absorption has a distinctive radial filamentary structure. This is probably the result of the superwind being driven by the starburst.

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