The Resolved Star Formation Rate in the Nearby Fireworks Galaxy: NGC6946

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We derive the spatially resolved star formation rate (SFR) for the face-on nearby galaxy NGC6946 by decomposing the radio emission from this galaxy into its thermal and non-thermal components. The decomposition utilized five radio maps from 3.5 cm to 22 cm that were convolved to a common angular resolution of 15 arcsec (500 pc). The derived free-free emission correlates well with the extinction corrected Hα emission. Model HII regions were used to derive the extinction-free number of ionizing photons and consequently the SFR.

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