Wilkins, S.M. and Gonzalez-Perez, V. and Lacey, C.G. and Baugh, C.M. (2012) 'Predictions for the intrinsic UV continuum properties of star-forming galaxies and the implications for inferring dust extinction.', Monthly notices of the Royal Astronomical Society., 424 (2). pp. 1522-1529.
The observed ultraviolet continuum (UVC) slope is potentially a powerful diagnostic of dust obscuration in star-forming galaxies. However, the intrinsic slope is also sensitive to the form of the stellar initial mass function and to the recent star formation and metal enrichment histories of a galaxy. Using the GALFORM semi-analytical model of galaxy formation, we investigate the intrinsic distribution of UVC slopes. For star-forming galaxies, we find that the intrinsic distribution of UVC slopes at z= 0, parametrized by the power-law index β, has a standard deviation of σβ≃ 0.30. This suggests an uncertainty on the inferred ultraviolet (UV) attenuation of Afuv≃ 0.7 (assuming a Calzetti attenuation curve) for an individual object, even with perfect photometry. Furthermore, we find that the intrinsic UVC slope correlates with star formation rate, intrinsic UV luminosity, stellar mass and redshift. These correlations have implications for the interpretation of trends in the observed UVC slope with these quantities irrespective of the sample size or quality of the photometry. Our results suggest that in some cases the attenuation by dust has been incorrectly estimated.
|Keywords:||Galaxies: formation, Ultraviolet: galaxies.|
|Full text:||(VoR) Version of Record|
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|Publisher Web site:||http://dx.doi.org/10.1111/j.1365-2966.2012.21344.x|
|Publisher statement:||This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS Published by Oxford University Press on behalf of Royal Astronomical Society. All rights reserved.|
|Date accepted:||No date available|
|Date deposited:||20 August 2014|
|Date of first online publication:||August 2012|
|Date first made open access:||No date available|
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