Gas and stellar dynamics in Stephan’s Quintet - Mapping the kinematics in a closely interacting compact galaxy group

Open Access

Table C.1.

continued.

CO	RA	Dec.	M_H₂ ^(b)
regions^(a)	(hh:mm:ss)	(dd:mm:ss)	(10⁸ M_⊙)
17	22:35:51.86	33:56:40.82
18_i	22:35:55.92	33:57:39.08	1.65 ± 0.18
18_ii	22:35:57.74	33:57:37.89	1.17 ± 0.15
18_iii	22:35:56.40	33:58:18.50	0.85 ± 0.17
18_iv	22:35:54.86	33:57:20.57
18a	22:35:56.71	33:57:55.58	1.47 ± 0.15
18b	22:35:58.32	33:57:55.58	3.10 ± 0.19
19_	22:36:02.59	33:58:46.56	9.62 ± 0.42
19_i	22:36:03.55	33:58:32.55	8.73 ± 0.43
19_ii	22:36:04.65	33:58:17.89	6.61 ± 0.34
19_iii	22:36:04.15	33:58:53.70	6.97 ± 0.48
19_iv	22:36:05.76	33:58:54.82	4.34 ± 0.42
19_v	22:36:05.21	33:58:38.54	6.28 ± 0.40
19_vi	22:36:06.60	33:58:26.69	1.93 ± 0.30
19_o	22:36:03.12	33:58:13.79	8.37 ± 0.43
b_i	22:36:01.58	33:58:02.08	8.84 ± 0.32
b_ii	22:36:01.56	33:58:23.30	6.57 ± 0.26
SF_i	22:35:59.54	33:58:34.60	6.32 ± 0.28
SF_ii	22:35:59.85	33:58:16.55	6.27 ± 0.24
SF_iii	22:35:59.85	33:58:04.00	5.45 ± 0.22
SF_iv	22:35:59.73	33:57:37.16	2.63 ± 0.29
SQ-A	22:35:58.88	33:58:50.69	4.64 ± 0.30

Notes.

^(a)

The CO regions have been extracted with 11″ radius circles from the smoothed CO maps.

^(b)

The H₂ gas mass obtained from integrating the spectra over the velocity range covering SQ (5100 − 7500 km/s).

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