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Paper: HST Observations of Star Formation in Interacting Galaxies: NGC 4194, the ``Medusa''
Volume: 240, Gas and Galaxy Evolution: A Conference in Honor of the 20th Anniversary of the VLA
Page: 210
Authors: Weistrop, D.; Eggers, D.; Nelson, C. H.; Kaiser, M. E.
Abstract: Ultraviolet and visible imaging of the blue compact galaxy NGC 4194 was obtained to survey the star-forming knots in the center of this galaxy. Photometry and image analysis were performed on these regions. Comparison with evolutionary tracks indicates many of the knots are reddened with a typical E(B-V)~0.3. The knot ages range from 3×106-108 years. Some of the knots may have masses 3-5×105 Msolar. The FUV fluxes correspond to the flux from 60-3.8×103 O5V stars.
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