A&A 461, 153 (2007)
DOI: 10.1051/0004-6361:20065002e

Erratum

Thermal and non-thermal components of the interstellar medium at sub-kiloparsec scales in galaxies

R. Paladino^1,2 - M. Murgia^1,3 - T. T. Helfer⁴ - T. Wong^5,6 - R. Ekers⁵ - L. Blitz⁴ - L. Gregorini^3,7 - L. Moscadelli¹

1 - INAF - Osservatorio Astronomico di Cagliari, Loc. Poggio dei Pini, Strada 54, 09012 Capoterra (CA), Italy
2 - Dipartimento di Fisica, Università di Cagliari, Cittadella Universitaria, 09042 Monserrato (CA), Italy
3 - Istituto di Radioastronomia - INAF, Via Gobetti 101, 40129 Bologna, Italy
4 - Radio Astronomy Laboratory, University of California, Berkeley, CA 94720, USA
5 - Australia Telescope National Facility, CSIRO, PO Box 76, Epping, N.S.W. 1710, Australia
6 - School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
7 - Dipartimento di Fisica, Università di Bologna, Via Irnerio 46, 40126 Bologna, Italy

A&A 456, 847-859 (2006), DOI: 10.1051/0004-6361:20065002

Key words: radio continuum: galaxies - galaxies: spiral - ISM: molecules - stars: formation - errata, addenda

Figure 7 published in A&A, 456 (2006) p. 856 is a duplicate of Fig. 8. Here, we provide the correct version of the figure. The change has no consequences for the discussion in the paper.

	Figure 1: RC-CO, RC-24 $\mu$m and 24 $\mu$m-CO correlations of NGC 7331, NGC 3627 and NGC 3521 at 6 arcsec resolution. The linear resolution achieved for each galaxy is indicated in the lower-right of the right-most panels.
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