Abstract
We have compared star formation rates and efficiencies, obtained from different star formation tracers, before and after compensation for internal extinction due to gas and dust, in the barred spiral galaxy M 83. The star formation tracers that we used were far-UV, B-band, radio thermal and non-thermal continuum, and Hα line emission. We calculated both SFRs and SFEs at 25′′ resolution. We use total gas map, derived from CO(J=1-0) and HI data to compensate for internal extinction.
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CITATION STYLE
Lundgren, A. A. (2008). Molecular gas and star formation in M 83. In Astrophysics and Space Science Proceedings (Vol. 0, p. 347). Springer Science and Business Media B.V. https://doi.org/10.1007/978-0-387-72768-4_83
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