The role of molecular gas in galaxy transition in compact groups

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Table 2

Molecular gas mass, SFR, and stellar mass.

Galaxy	Distance^a	log(M_mol,0)^b	log(M_mol)^b	Ref. ^d	SFR ^e	log(M_∗)^f
	[Mpc]	[M_⊙]	[M_⊙]		[M_⊙ yr^-1]	[M_⊙]

HCG01b	146.6	9.23	9.35	1	0.63	10.61
HCG02b	62.1	8.92	9.19	4	6.08	9.65
HCG04a	114.9	10.09	10.49	4	23.45	10.49
HCG05a	174.0	9.99	10.24	1	1.60	10.99
...	...	...	...	...	...	...

Notes. The full table is available at the CDS.

^(b)

Distance derived from redshift with H₀ = 70 km s^-1 Mpc^-1.

^(b)

Cold molecular gas within the central pointing, calculated from Eq. (2).

^(c)

Cold molecular gas mass, extrapolated from the central pointing to the entire disk, calculated as described in Sect. 2.2.

^(d)

References for the CO(1−0) measurements: (1) this work; (2) Lisenfeld et al. (2014); (3) Martinez-Badenes et al. (2012); (4) Leon et al. (1998); (5) Verdes-Montenegro et al. (1998); (6) Wiklind et al. (1995); and (7) Mirabel et al. (1990).

^(e)

Star formation rate, calculated from the WISE W4 band with Eq. (4).

^(f)

Stellar mass, calculated from the WISE W1 and W2 bands with Eq. (5).

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