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A&A 424, 465-476 (2004)
DOI: 10.1051/0004-6361:20047024
The radial extinction profiles of late-type galaxies
S. Boissier1, A. Boselli2, V. Buat2, J. Donas2 and B. Milliard21 Carnegie Observatories, 813 Santa Barbara Street, Pasadena, 91101 California, USA
e-mail: boissier@ociw.edu
2 Laboratoire d'Astrophysique de Marseille, Traverse du siphon, 13376 Marseille Cedex 12, France
e-mail: [Alessandro.Boselli;Veronique.Buat;Jose.Donas;Bruno.Milliard]@oamp.fr
(Received 7 January 2004 / Accepted 13 May 2004 )
Abstract
We have used UV (FOCA) and FIR (IRAS) images of six nearby late
type galaxies to study the radial variation of the UV extinction
(deduced from the FIR/UV ratio). We compare the UV extinction
gradient with other extinction indicators (Balmer decrement) and
search for a relation between the extinction, the metallicity and
the gas surface density among our galaxies. We detect in our small
sample a clear relation between extinction and metallicity.
These observed relations are used to calibrate an
empirical recipe useful for extinction correction in the UV,
visible and near-infrared images of late type galaxies.
Key words: galaxies: spiral -- ultraviolet: galaxies -- ISM: dust, extinction
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© ESO 2004
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