UVOT measurements of dust and star formation in the SMC and M33

Lea M.Z. Hagen, Michael Siegel, Caryl Gronwall, Erik Hoversten, Angelica Vargas, Stefan Immler

Research output: Contribution to journalConference article

Abstract

When measuring star formation rates using ultraviolet light, correcting for dust extinction is a critical step. However, with the variety of dust extinction curves to choose from, the extinction correction is quite uncertain. Here, we use Swift/UVOT to measure the extinction curve for starforming regions in the SMC and M33. We find that both the slope of the curve and the strength of the 2175 Å bump vary across both galaxies. In addition, as part of our modeling, we derive a detailed recent star formation history for each galaxy.

Original languageEnglish (US)
Article number140
JournalProceedings of Science
StatePublished - Jan 1 2014
Event10th Conference on Swift, SWIFT 2014 - Rome, Italy
Duration: Dec 2 2014Dec 5 2014

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All Science Journal Classification (ASJC) codes

  • General

Cite this

Hagen, L. M. Z., Siegel, M., Gronwall, C., Hoversten, E., Vargas, A., & Immler, S. (2014). UVOT measurements of dust and star formation in the SMC and M33. Proceedings of Science, [140].