TY  - GEN 
AU  - Lisenfeld , Ute
AU  - Espada Fernández, Daniel
AU  - Verdes-Montenegro, L.
AU  - Kuno, N.
AU  - Leon, S.
AU  - Sabater, J.
AU  - Sato, N.
AU  - Sulentic, J.
AU  - Verley, Simon
AU  - Yun, M. S.
PY  - 2011
SN  - 0004-6361
SN  - 1432-0746
SN  - doi: 10.1051/0004-6361/201117056
UR  - http://hdl.handle.net/10481/28373
AB  - Aims. We characterize the molecular gas content (ISM cold phase) using CO emission of a redshift-limited subsample of isolated galaxies from the AMIGA (Analysis of the interstellar Medium of Isolated GAlaxies) project in order to provide a comparison...
AB  - Methods. We present the 12CO(1–0) data for 273 AMIGA galaxies, most of them (n = 186) from our own observations with the IRAM 30 m and the FCRAO 14 m telescopes and the rest from the literature. We constructed a redshift-limited sample containing...
AB  - Results. We find correlations between MH2 and LB, , LK, and LFIR. The tightest correlation of MH2 holds with LFIR and, for T = 3–5, with LK, and the poorest with . The correlations with LFIR and LK are very close to linearity. The correlation with LB...
LA  - eng
PB  - European Southern Observatory (ESO); Springer Verlag
KW  - Galaxies
KW  - Evolution
KW  - Interactions
KW  - ISM
KW  - Radio lines
KW  - Surveys
TI  - The AMIGA sample of isolated galaxies IX. Molecular gas properties
ER  -