Molecular gas in super spiral galaxies | Astronomy & Astrophysics (A&A)

Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/202449493e]

Table 1.

Velocity-integrated CO intensities (central pointings).

Galaxy name	rms ^(a)	I_{CO(1 − 0)}^(b)	det ^(c)	ΔV_{CO(1 − 0)}^(d)
	[mK]	[K km s⁻¹]		[km s⁻¹]
2MFGC12344	0.88	1.57 ± 0.13	0	1018
OGC 139	1.67	< 0.60	1	700
OGC 217	1.67	1.39 ± 0.14	0	347
OGC 290	1.46	1.02 ± 0.13	0	403
...	...	...	...	...

Notes.

^(a)

Root-mean-square noise at a velocity resolution of 40 km s⁻¹.

^(b)

Velocity integrated intensity and statistical error of the CO(1–0) line.

^(c)

Detection code: 0 = detection (S/N ≳ 5), 2 = tentative detection (S/N ≈ 3 − 5), 1 = nondetection.

^(d)

Zero-level line width. The uncertainty is roughly given by the velocity resolution (∼20 km s⁻¹).

The full table is available online at the CDS.

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