Relics of an eruptive starburst in NGC 1569

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Galactic Evolution, Galactic Structure, Irregular Galaxies, Star Formation, Starburst Galaxies, Charge Coupled Devices, Emission Spectra, Galactic Nuclei, H Alpha Line, H Ii Regions, Spectral Line Width

Scientific paper

H-alpha, R, and I band CCD images of the 'posteruptive' irregular galaxy NGC 1569 are presented. The discovery of two archlike structures of diffuse H-alpha emission located more than 1 kpc beyond the star-forming bar is reported. These features are used to estimate an age for the near-nuclear starburst that created them along with other filamentary and armlike structures previously seen in H-alpha photographs. The gravitational and kinematic energies associated with the H-alpha arcs are estimated to be orders of magnitude higher than can be provided by a single supernova explosion. Coherent outbursts involving thousands of supernovae each could explain the diffuse H-alpha features without exceeding the starbirth rate inferred from the total H-alpha luminosity of the galaxy.

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