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Table 1

Results of the CO observations on our sample of ETGs.

12CO(1–0) 12CO(2–1)
Galaxy name V Telescope FCO Δv rms Profile FCO Δv rms MH2 CO ratio
km s-1 K km s-1 km s-1 mK K km s-1 s-1 mK 108 M

UGC 0968 2379 IRAM 3.45 ± 0.58 430 7.2 dh 5.9 ± 1.2 430 10 1.48 ± 0.25 0.60 ± 0.2
UGC 5617 1151 IRAM 1.40 ± 0.40 304 5.9 sp 3.03 ± 0.37 300 3.8 0.31 ± 0.09 0.75 ± 0.2
UGC 6860 1259 NRO <9.4 11.0 <0.85
UGC 6946 1040 IRAM <4.8 4.1 <1.2 3.7 <0.71
UGC 6946 1040 NRO 2.5 ± 0.7 187 9.0 dh 0.17 ± 0.05
UGC 7203 2215 IRAM <4.5 4.5 <1.4 4.6 <2.95
UGC 8355 2778 NRO 2.3 ± 0.7 240 8.2 sp 0.91 ± 0.28
UGC 8499 2533 NRO <10.5 14.9 <3.6
UGC 9706 1714 IRAM <4.3 3.7 <2.9 7.3 <1.6

Notes. Column description: (1) name; (2) recession velocity; (3) telescope used for the observation; CO(1–0) observations: (4) integrated line emission in K km s-1; (5) velocity width; (6) rms of the spectrum in mK; (7) shape of the line profile: dh (double-horn), sp (single peak); CO(2–1) observations: (8) integrated line emission in K km s-1; (9) spectral region of integration; (10) rms of the spectrum in mK; (11) evaluation of H2 mass from CO(1–0) line intensity; (12) CO(2–1)/CO(1–0) ratio.

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