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Issue A&A
Volume 424, Number 2, September III 2004
Page(s) 465 - 476
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20047024



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. Milliard2

1  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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