Spatially resolved gas and stellar kinematics in compact starburst galaxies

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Volume 666 (October 2022)

A&A, 666 (2022) A161

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Table 7.

Spatially resolved measurements.

Name	Class ^(a)	v_shear	v_rot	σ_m	v_shear/σ_m	σ_m, corr	v_rot/σ_m, corr
		(km s⁻¹)	(km s⁻¹)	(km s⁻¹)
J0018−0903	CK	18.2 ± 1.6	99.6 ± 41.2	44.5 ± 6.6	0.41 ± 0.07	43.0 ± 6.5	2.31 ± 1.02
J0230−0720	PR	61.4 ± 0.3	88.1 ± 1.0	46.5 ± 3.6	1.32 ± 0.10	44.6 ± 3.5	1.98 ± 0.16
J1140−0024	CK	18.4 ± 2.0	20.8 ± 2.3	43.3 ± 9.4	0.43 ± 0.10	43.1 ± 9.4	0.48 ± 0.12
J1155−0100	PR	55.7 ± 0.5	125.8 ± 4.7	44.7 ± 4.5	1.25 ± 0.12	43.8 ± 4.4	2.87 ± 0.31
J1211+1424	RD	132.6 ± 0.6	139.6 ± 0.6	75.2 ± 7.8	1.76 ± 0.18	69.2 ± 7.2	2.01 ± 0.21
J1336+0748	CK*	30.3 ± 1.7	36.0 ± 2.0	42.1 ± 8.3	0.72 ± 0.15	41.2 ± 8.2	0.88 ± 0.18
J1339−0045	CK*	19.1 ± 2.2	21.5 ± 2.4	34.0 ± 6.6	0.56 ± 0.12	31.7 ± 6.4	0.68 ± 0.16
J1340+0616	M*	57.9 ± 2.2	62.7 ± 2.4	54.4 ± 9.6	1.06 ± 0.19	50.5 ± 9.1	1.24 ± 0.22
J1353−0231	M	119.3 ± 0.9	137.0 ± 1.1	125.3 ± 8.2	0.95 ± 0.06	118.5 ± 7.8	1.15 ± 0.08
J1400+0404	RD	128.1 ± 0.2	219.4 ± 2.6	52.3 ± 4.5	2.45 ± 0.21	44.9 ± 3.9	4.89 ± 0.43
J1412−0049	M*	28.4 ± 1.3	38.1 ± 1.7	37.8 ± 6.5	0.76 ± 0.13	36.2 ± 6.3	1.05 ± 0.19
J1513+0431	PR*	35.0 ± 2.0	37.6 ± 2.2	45.3 ± 6.1	0.77 ± 0.11	43.1 ± 5.9	0.87 ± 0.13
J1525+0500	PR	143.9 ± 0.6	171.5 ± 0.9	55.8 ± 8.7	2.58 ± 0.40	48.5 ± 7.8	3.53 ± 0.56
J1545+0814	M	97.1 ± 1.3	107.5 ± 1.5	82.6 ± 9.1	1.18 ± 0.13	79.8 ± 8.8	1.35 ± 0.15
J2256+1305	PR*	29.2 ± 1.7	31.5 ± 1.8	48.1 ± 8.5	0.61 ± 0.11	47.7 ± 8.5	0.66 ± 0.12

Notes.

^(a)

Galaxy classification: RD: rotating disks, PR: perturbed rotators, CK: complex kinematics, M: mergers, evidence for interacting (see text). The sources denoted with a star have only part of the galaxy covered with ionised gas, so it is hard to see the entire galaxy kinematics.

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