The AMIGA sample of isolated galaxies (Corrigendum)
IX. Molecular gas properties
U. Lisenfeld1,2, D. Espada3,4, L. Verdes-Montenegro3, N. Kuno5, S. Leon6, J. Sabater7, N. Sato8, J. Sulentic3, S. Verley1 and M. S. Yun9
1 Departamento de Física Teórica y del Cosmos, Universidad de Granada, 18071 Granada, Spain
e-mail: ute@ugr.es
2 Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada, Spain
3 Instituto de Astrofísica de Andalucía (CSIC) Apdo. 3004, 18080 Granada, Spain
4 National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
5 Nobeyama Radio Observatory, Minamimaki, Minamisaku, Nagano 384-1805, Japan
6 Joint Alma Observatory/ESO, Las Condes, Santiago, Chile
7 Institute for Astronomy, University of Edinburgh, Edinburgh EH9 3HJ, UK
8 Student Center for Independent Research in the Science, Wakayama University, 930 Sakaedani, Wakayama, 640-8510, Japan
9 Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA
Key words: galaxies: evolution / galaxies: ISM / galaxies: interactions / radio lines: ISM / radio lines: galaxies / errata, addenda
We noticed two errors in our paper: (1) in Eqs. (6) and (7) the units for LIR and LFIR should be erg s-1 (instead of erg yr-1). (2) In Table 8 there are some erroneous values for the means of the AMIGA sample (i.e. in Cols. 2 and 3). None of these errors affect the conclusions of the paper. Below we attach the correct version of the table.
Mean deficiencies of MH2, LFIR and LFIR/MH2 in interacting samples and AMIGA.
© ESO, 2012
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