Authors: S. A. Eales, M. W. L. Smith, C. D. Wilson, G. J. Bendo, L. Cortese, M. Pohlen, A. Boselli, H. L. Gomez, R. Auld, M. Baes, M. J. Barlow, J. J. Bock, M. Bradford, V. Buat, N. Castro-Rodríguez, P. Chanial, S. Charlot, L. Ciesla, D. L. Clements, A. Cooray, D. Cormier, J. I. Davies, E. Dwek, D. Elbaz, M. Galametz, F. Galliano, W. K. Gear, J. Glenn, M. Griffin, S. Hony, K. G. Isaak, L. R. Levenson, N. Lu, S. Madden, B. O'Halloran, K. Okumura, S. Oliver, M. J. Page, P. Panuzzo, A. Papageorgiou, T. J. Parkin, I. Pérez-Fournon, N. Rangwala, E. E. Rigby, H. Roussel, A. Rykala, N. Sacchi, M. Sauvage, B. Schulz, M. R. P. Schirm, L. Spinoglio, S. Srinivasan, J. A. Stevens, M. Symeonidis, M. Trichas, M. Vaccari, L. Vigroux, H. Wozniak, G. S. Wright and W. W. Zeilinger.<br />Astronomy and Astrophysics Vol. 518 , page L62<br />Published online: 16/07/2010<br />
Keywords:
galaxies: ISM ; galaxies: spiral ; dust, extinction ; ISM: abundances .
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