Deciphering the imprint of active galactic nucleus feedback in Seyfert galaxies - Nuclear-scale molecular gas deficits

Open Access

Table C.1.

Gas surface densities and concentration indices in the galaxies of our combined sample.

Name	D	log $_{10} Σ_{50}^{gas}$ $_{10} \Sigma^{\mathrm{gas}}_{50}$	log $_{10} Σ_{200}^{gas}$ $_{10} \Sigma^{\mathrm{gas}}_{200}$	CCI	log $_{10} Σ_{50}^{hot}$ $_{10} \Sigma^{\mathrm{hot}}_{50}$	log $_{10} Σ_{200}^{hot}$ $_{10} \Sigma^{\mathrm{hot}}_{200}$	HCI

—-	Mpc	M_⊙pc⁻²	M_⊙pc⁻²	—-	M_⊙pc⁻²	M_⊙pc⁻²	—-
AGN sample: CO(3-2)

NGC1566	7.2	2.58	1.89	0.69	-3.10	-3.54	0.44
NGC1808	9.3	2.68	2.20	0.48	-2.83	-3.23	0.40
NGC1672	11.4	3.16	2.22	0.83	-2.65	-3.20	0.55
NGC1068	14.0	2.69	2.94	-0.25	-1.41	-1.61	0.20
NGC6300	14.0	3.09	2.42	0.68	-3.19	-3.93	0.74
NGC1326	14.9	2.51	1.77	0.74	-2.79	-3.47	0.68
NGC5643	16.9	3.17	2.61	0.56	-2.54	-3.38	0.85
NGC613	17.2	3.22	2.51	0.82	-1.81	-2.65	0.85
NGC7314	17.4	2.22	1.53	0.69	—	—	—
NGC4388	18.1	1.97	2.13	-0.17	-2.47	-2.64	0.17
NGC1365	18.3	2.22	1.52	0.70	-4.91	-4.18	-0.73
NGC4941	20.5	2.21	1.42	0.79	—	—	—
NGC7213	22.0	< 1.18	0.63	< 0.55	-2.98	-3.87	0.89
NGC7582	22.5	2.77	2.93	-0.16	-3.35	-3.53	0.18
NGC6814	22.8	1.66	0.96	0.70	-2.35	-3.21	0.86
NGC3227	23.0	2.88	2.74	0.14	-2.60	-3.11	0.50
NGC5506	26.4	2.42	2.34	0.07	-2.03	-2.47	0.43
NGC7465	27.2	2.65	2.07	0.57	-2.28	-2.78	0.50
NGC7172	37.0	1.81	1.97	-0.16	-5.53	-5.68	0.15
NGC5728	44.5	2.65	2.55	0.10	-4.86	-5.31	0.45

AGN sample: CO(2-1)

NGC4826	4.4	2.67	2.28	0.39	-2.92	-3.19	0.27
NGC5236	4.9	2.87	2.62	0.25	—	—	—
NGC2903	10.0	2.40	2.31	0.09	—	—	—
NGC3351	10.0	2.52	2.21	0.32	-3.31	-3.77	0.46
NGC1637	11.7	2.68	2.20	0.48	—	—	—
NGC4569	16.8	2.41	2.31	0.10	-2.90	-2.84	-0.06
NGC4579	16.8	1.76	1.45	0.32	-1.89	-2.62	0.73
NGC3718	17.0	1.26	0.80	0.46	—	—	—
NGC2110	34.8	< 1.39	1.41	< − 0.02	-5.09	-5.32	0.23
NGC2782	35.0	2.77	2.34	0.42	—	—	—
NGC7172	37.0	2.07	2.16	-0.08	-5.53	-5.68	0.15
MCG-06-30-15	38.3	2.27	2.05	0.22	-3.33	-3.38	0.05
NGC2992	39.2	1.70	1.99	-0.30	-5.73	-5.79	0.06
NGC3081	40.3	2.03	1.88	0.14	-5.84	-5.75	-0.09
ESO137-34	41.5	2.42	2.21	0.21	-2.21	-2.45	0.24
NGC5728	44.5	2.68	2.64	0.04	-4.86	-5.31	0.45
ESO21-g004	45.1	1.70	1.57	0.13	—	—	—
NGC4826	4.4	2.71	2.23	0.47	-2.92	-3.19	0.27
NGC3351	10.0	2.50	1.91	0.55	-3.31	-3.57	0.46
NGC4501	14.0	2.73	2.36	0.37	-2.88	-3.09	0.21
NGC4438	16.5	2.75	2.49	0.25	-1.87	-2.38	0.51
NGC3368	18.0	2.93	2.67	0.25	-2.48	-2.94	0.46
NGC7172	37.0	2.10	2.16	-0.06	-5.53	-5.68	0.15

AGN sample: CO(1-0)

M51	8.6	2.84	2.18	0.66	—	—	—
NGC6300	14.0	3.48	2.64	0.84	-3.19	-3.93	0.74
NGC4321	16.8	3.35	2.91	0.44	—	—	—
NGC5643	16.9	2.75	2.38	0.37	-2.54	-3.38	0.85
NGC7314	17.4	2.86	2.31	0.55	—	—	—
NGC4388	18.1	2.31	2.43	-0.12	-2.47	-2.64	0.17
NGC6221	22.9	3.33	3.03	0.30	—	—	—
NGC3227	23.0	< 2.33	2.49	< − 0.15	-2.60	-3.11	0.50
NGC4180	36.0	3.22	2.79	0.43	—	—	—
NGC7172	37.0	2.69	2.72	-0.04	-5.53	-5.68	0.15
NGC4593	41.8	2.78	2.65	0.14	-4.85	-5.65	0.80
NGC1125	42.6	< 2.79	2.60	< 0.19	—	—	—
NGC5728	44.5	2.99	3.05	-0.06	-4.86	-5.31	0.45
NGC3281	52.0	3.00	2.89	0.10	-2.29	-2.38	0.09

nonAGN sample: CO(2-1)

NGC5068	5.2	0.75	0.29	0.46	—	—	—
NGC3621	7.1	0.68	0.54	0.14	—	—	—
IC5332	9.0	0.25	-0.01	0.25	—	—	—
NGC3596	11.3	1.67	1.58	0.09	—	—	—
NGC4781	11.3	1.38	1.11	0.27	—	—	—
NGC2835	12.2	1.24	0.99	0.25	—	—	—
NGC5530	12.3	1.54	1.13	0.41	—	—	—
NGC1947	17.2	3.46	2.70	0.76	—	—	—
NGC1079	18.9	2.12	1.63	0.48	—	—	—
NGC3717	19.1	2.88	2.49	0.39	—	—	—
NGC7727	21.0	2.36	2.02	0.34	-2.97	-3.45	0.48
NGC5921	21.0	2.73	2.26	0.47	—	—	—
NGC3175	21.0	2.67	2.50	0.17	-3.30	-3.55	0.25
NGC718	21.4	2.18	1.78	0.41	-2.98	-3.77	0.79
NGC5845	27.0	1.73	1.01	0.62	—	—	—
ESO-093-g003	29.8	1.97	1.99	-0.02	—	—	—
NGC5037	35.0	2.59	2.34	0.25	—	—	—
NGC3749	41.0	2.84	2.63	0.20	—	—	—
NGC4224	41.0	1.86	1.70	0.16	—	—	—

Notes. Columns (3) and (4) list the surface densities of the cold molecular derived from different CO lines on the nuclear (r ≤ 50 pc; $Σ_{50}^{gas}$ $\Sigma^{\mathrm{gas}}_{50}$ ) and circumnuclear (r ≤ 200 pc; $Σ_{200}^{gas}$ $\Sigma^{\mathrm{gas}}_{200}$ ) disk scales of the AGN and nonAGN galaxies of the sample. The target names and their distances are listed in columns (1) and (2). The concentration indices of cold molecular gas (CCI) are listed in column (5). Columns (6), (7) and (8) list the corresponding surface densities and concentration indices ( $Σ_{50}^{hot}$ $\Sigma^{\mathrm{hot}}_{50}$ , $Σ_{200}^{hot}$ $\Sigma^{\mathrm{hot}}_{200}$ , and HCI) derived for the hot molecular gas component.

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