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Table 6

Environmental characteristics of UGC 11919 and NGC 6824.

# Object designation RA Dec cz H I flux (Jy   km   s-1) V lg MH   I (109   M) MH   I/LB
(1) (2) (3) (4) (5) (6) (7) (8) (9)

UGC 11919

1 UGC 11927 22:09:27.86 +40:59:56.7 4501 7.46 4800 7.21 0.43
2 22:07:30.80 +41:01:55.4 4398 0.44 4698 0.4
3 22:07:17.93 +41:06:00.1 4448 1.16 4747 1.09
4 2MASX J22094543+4112200 22:09:43.18 +41:12:38.5 4536 4.78 4836 4.69
5 22:07:36.15 +41:47:26.8 4388 1.15 4688 1.06
6 CGCG 530-014 22:10:34.14 +40:54:37.7 4525 18.03 4824 17.6 0.81
7 UGC 11925 22:09:10.35 +41:24:41.1 4548 0.97 4848 0.96 0.16
8 NGC 7223 22:10:08.31 +41:01:12.0 4697 18.4 4997 19.3 0.3
9 22:09:26.87 +41:05:31.7 4465 0.36 4765 0.34
10 22:09:25.16 +41:08:51.8 4568 0.4 4868 0.4
11 22:10:26.16 +40:59:44.6 4647 7.62 4947 7.83
12 22:07:48.81 +41:22:01.3 4620 1.43 4920 1.45
13 2MASX J22090972+4115259 22:09:09.99 +41:15:26.7 4772 1.97 5072 2.12
14 22:07:35.56 +41:18:57.7 4693 1.04 4993 1.09
15 22:10:12.18 +41:35:17.2 4703 1.77 5003 1.86
16 UGC 11919 22:08:10.51 +41:10:47.4 5354 7.17 5654 9.61 0.3
17 LEDA 3087958 22:09:36.12 +41:16:52.6 5447 0.45 5747 0.63 0.07
18 22:08:15.09 +41:42:28.9 5499 3.23 5799 4.56
19 22:09:51.82 +41:27:48.0 5499 0.88 5799 1.24
20 CGCG 530-011 22:08:12.18 +41:16:19.6 5709 4.63 6009 7.01 0.35
21 22:07:48.03 +41:12:45.0 5606 0.23 5906 0.34
22 22:07:43.38 +41:43:25.6 5735 0.51 6035 0.78

NGC 6824

1 NGC 6824 19:43:41.27 +56:06:34.0 3563 1.88 3835 1.16 0.02
2 19:44:04.82 +56:29:03.9 3493 0.74 3766 0.44
3 LEDA 214725 19:43:57.39 +56:04:33.9 3949 0.16 4221 0.12 0.16
4 19:43:29.69 +55:50:22.7 4164 0.18 4436 0.15

Notes. (1) Number of detected object, as labeled in Fig. 13; (2) Name of object if known; (3) Right ascension J2000; (4) Declination J2000; (5) Optical recession velocity; (6) Total H I flux F in Jy   km   s-1; (7) Velocity corrected to the centroid of the Local Group using the formula following Yahil et al. (1977); (8) H I total mass calculated from the total flux via M = 2.36 × 105(Vlg/(75km   s-1))2F; (9) H I mass-to-light ratio, the B-band magnitudes were taken from Hyperleda. Galaxies with the velocities lying at the edge of the observed data cube (so the systemic velocity is uncertain for them) are marked by asterisks.

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