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Attenuation Caused by a Distant Isothermal Turbulent Screen

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© 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Jörg Fischera and Michael Dopita 2005 ApJ 619 340 DOI 10.1086/426185

0004-637X/619/1/340

Abstract

We analyze in detail the attenuation caused by an isothermal turbulent distant foreground dust screen. The attenuation curve is well determined by two parameters, the absolute-to-relative attenuation ratio R = AV/E(B - V) and the absolute attenuation AV. We show quantitatively how these two observable quantities depend on the statistical properties of the local density and the mean attenuation ⟨AV⟩ and how they vary with the thickness of the screen measured in units of the largest turbulent scale. The attenuation through a turbulent medium is characterized by higher transparency and a flatter attenuation curve in comparison with a homogeneous dust screen. In general, the effect of a turbulent medium on the attenuation increases with slice thickness. In the limit of thick slices, typically larger than the maximum turbulent scale, R asymptotically approaches a maximum value.

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10.1086/426185