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Table 4

CO measurements.

Galaxy VCO ΔVCO TA,1−0 TA ∗ ,2−1 δ Trms,1−0 δ Trms,2−1 ICO,1−0 ICO,2−1 log LCO log ΣH2
km s-1 km s-1 mK mK mK mK K km s-1 K km s-1 K km s-1 pc2 M pc-2
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)

Haro 1 3793.0 ± 6 151 73.6 76.0 8.9 12.0 15.1 ± 0.5 19.4 ± 0.8 8.7 1.81
Mrk 33 1482.5 ± 8 85 43.5 46.3 7.0 4.9 4.6 ± 0.3 6.7 ± 0.5 7.4 1.14
Mrk 35 939 ± 6 90 23.6 37.0 5.0 9.2 2.3 ± 0.2 2.0 ± 0.3 6.8 0.85
Mrk 36 646 ± 7 ... ... ... 4.7 5.0 <0.4 <0.6 <5.7 <0.10
Mrk 297 4731 ± 5 127 97.7 115 7.2 9.2 19.2 ± 0.6 27.3 ± 0.2 9.0 1.81
Mrk 314 2091 ± 6a 161a ... 5.4 5.6 2.7 <0.6 1.7 6.7a 0.13a
Mrk 324 1600 ± 6 ... ... ... 5.6 5.3 <0.7 <0.9 <6.6 <0.39
Mrk 401 1699 ± 6 43 148.6 169.1 6.6 9.1 8.6 ± 0.3 15.2 ± 0.5 7.8 1.46
III Zw 102 1615 ± 4 130 203.7 201.4 15.3 20.7 40.0 ± 0.4 38.3 ± 0.5 8.4 2.23
III Zw 107 5785 ± 11 120 3.7 7.8 2.0 2.6 0.6 ± 0.3 0.7 ± 0.2 7.7a 0.24a

Notes. Columns: (2) and (3) CO 10 line central LSR velocity and width at half maximum; (4), (5) and (6), (7) peak intensity and rms of CO 1  0 and CO 2  1 lines, respectively; (8) and (9) integrated line emission and 1σ error bars in Tmb units (Icodv). 3σ upper limits are given for non-detections; (10) and (11) CO (11) luminosity and H2 surface brightness assuming a Galactic CO-to-H2 conversion factor. . Its integrated flux was converted to CO 10 flux to derive the values in (10) and (11).

(a)

It corresponds to the 21 line, which is detected at ~3σ

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