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Table 2

CO mapping over the bright UV region at 1.36 r25.

CO(1–0) CO(2–1)
Offsets Time rmsa FWHM b F c rmsa FWHM b F c r 2,1 d M H2 e ΣH2 f
() () (min) (mK) (kms-1) (K km s-1) (mK) (kms-1) (K km s-1) (106M) (M pc2)

−66 0 118 5 10 <0.15 6 10 <0.18 <0.97 <0.38
−66 +22 117 5 11 0.14 ± 0.06‡ 6 10 <0.18 <0.39 0.90 ± 0.39 0.35 ± 0.15
−44 0 186 4 10 <0.12 4 10 <0.12 <0.78 0.30
−44 +22 164 4 10 <0.12 6 10 <0.18 <0.78 0.30
−22 0 171 4 14 0.21 ± 0.06 5 10 <0.15 <0.22 1.36 ± 0.39 0.53 ± 0.15
−22 +22 148 4 10 <0.12 6 10 <0.18 <0.78 <0.30
0 0 164 4 10 <0.12 5 10 <0.15 <0.78 <0.30
0 +22 148 5 10 <0.15 6 10 <0.18 <0.97 <0.38
+22 0 123 5 10 <0.15 7 10 <0.21 <0.97 <0.38
+22 +22 116 5 10 <0.15 8 10 <0.24 <0.97 <0.38
+44 0 63 7 10 <0.21 9 10 <0.27 <1.36 <0.53
+44 +22 62 7 10 <0.21 8 10 <0.24 <1.36 <0.53
All offsets 1932 1 23 0.11 ± 0.02 2 10 <0.06 <0.17 0.71 ± 0.13 0.28 ± 0.05

Notes. The last separate line gives the values obtained when summing all scans at the 12 offset pointings.

(a)

Rms noises at, respectively, 3 mm and 1 mm, measured per channel of 3.2 km s-1 and 1.3 km s-1.

(b)

Full widths at half maximum of, respectively, CO(1–0) and CO(2–1) lines as determined from fitting Gaussian profiles.

(c)

Integrated CO(1–0) and CO(2–1) line fluxes as determined from fitting Gaussian profiles. The value marked with corresponds to a potentially less reliable measurement, because of the CO line detection at barely 3σ. Upper limits are 3σ and are calculated assuming a 10 km s-1 line width.

(d) +(e) +(f)

CO luminosity ratios, H2 masses, and H2 surface densities, respectively, calculated using the same prescriptions as in Table 1.

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