Star-Forming or Starbursting? The Ultraviolet Conundrum
M. Boquien, D. Calzetti, R. Kennicutt, D. Dale, C. Engelbracht, K. D., Gordon, S. Hong, J. C. Lee, J. Portouw

TL;DR
This study investigates the causes of dispersion in the IRX-beta diagram for star-forming regions, finding that dust geometry and extinction laws are key factors, with implications for understanding galaxy dust attenuation.
Contribution
The paper provides new insights into the causes of IRX-beta dispersion by analyzing individual star-forming regions and highlighting the role of dust properties and geometries.
Findings
Dispersion not correlated with stellar age.
Range of dust geometries and extinction curves cause dispersion.
Positive correlation between dust attenuation and metal content.
Abstract
Compared to starburst galaxies, normal star forming galaxies have been shown to display a much larger dispersion of the dust attenuation at fixed reddening through studies of the IRX-beta diagram (the IR/UV ratio "IRX" versus the UV color "beta"). To investigate the causes of this larger dispersion and attempt to isolate second parameters, we have used GALEX UV, ground-based optical, and Spitzer infrared imaging of 8 nearby galaxies, and examined the properties of individual UV and 24 micron selected star forming regions. We concentrated on star-forming regions, in order to isolate simpler star formation histories than those that characterize whole galaxies. We find that 1) the dispersion is not correlated with the mean age of the stellar populations, 2) a range of dust geometries and dust extinction curves are the most likely causes for the observed dispersion in the IRX-beta diagram…
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Taxonomy
TopicsHistory and Developments in Astronomy · Astro and Planetary Science · Solar and Space Plasma Dynamics
