Table 5
Group 7: Serendipity and literature.
Number | Name | RA (J2000) | Dec (J2000) | Ref. | WISE | Figure | Comments |
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G7-01 | M17-S1 | 18:20:22.72 | −16:08:34.27 | A | • | − | M17 region |
G7-02 | M17-S2 | 18:20:25.88 | −16:08:32.48 | A | • | − | M17 region |
G7-03 | M17-S3 | 18:20:26.63 | −16:07:08.55 | A | • | − | M17 region |
G7-04 | RCW 49-S1 | 10:22:23.06 | −57:44:27.92 | A | ⊃ | Fig. 7 | RCW 49 region |
G7-05 | RCW 49-S2 | 10:24:03.12 | −57:48:36.00 | A | • | − | RCW 49 region |
G7-06 | RCW 49-S3 | 10:24:39.18 | −57:45:20.97 | A | • | − | RCW 49 region |
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G7-07 | K1 | 20:34:28.9 | +41:56:17.0 | B | ⊃ | Fig. 7 | Cygnus-X region |
G7-08 | K2 | 20:34:34.5 | +41:58:29.3 | B | ⊃ | Fig. 7 | Cygnus-X region |
G7-09 | K3 | 20:28:30.2 | +42:00:35.2 | B | ⊃ | Fig. 7 | Cygnus-X region |
G7-10 | K4 | 20:28:39.4 | +40:56:51.0 | B | ⊃ | Fig. 7 | Cygnus-X region |
G7-11 | K5 | 20:34:55.1 | +40:34:44.0 | B | ⊃ | Fig. 7 | Cygnus-X region |
G7-12 | K6 | 20:36:13.3 | +41:34:26.1 | B | ⊃ | Fig. 8 | Cygnus-X region |
G7-13 | K7 | 20:36:04.4 | +40:56:13.0 | B | ⊃ | Fig. 8 | Cygnus-X region |
G7-14** | K8 | 20:20:11.6 | +39:45:30.1 | B | ? | − | Cygnus-X region, Special case |
G7-15** | K9 | 20:25:43.9 | +38:11:13.2 | B | ? | − | Cygnus-X region, Special case |
G7-16 | K10 | 20:29:22.1 | +37:55:44.3 | B | ⊃ | Fig. 8 | Cygnus-X region |
G7-17* | K11 | 20:33:36.1 | +43:59:07.4 | B | ⊃ | Fig. 8 | Cygnus-X region, BD +43° 3654 |
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G7-18 | G1 | 17:27:11.23 | −34:14:34.9 | C | ⊃ | Fig. 8 | NGC 6357 region |
G7-19 | G2 | 17:22:03.43 | −34:14:24.1 | C | ⊃ | Fig. 8 | NGC 6357 region |
G7-20** | G3 | 17:28:21.67 | −34:32:30.3 | C | ⊃ | Fig. 9 | NGC 6357 region, HD 319881 |
G7-21** | G4 | 17:18:15.40 | −34:00:06.1 | C | ⊃ | Fig. 9 | NGC 6357 region, New RGB figure |
G7-22 | G5 | 17:22:05.62 | −35:39:55.5 | C | ⊃ | Fig. 9 | NGC 6357 region, [N78] 34 |
G7-23** | G6 | 17:22:50.02 | −34:03:22.4 | C | ⊃ | Fig. 9 | NGC 6357 region |
G7-24 | G7 | 17:27:12.53 | −33:30:40.0 | C | ⊃ | Fig. 9 | NGC 6357 region |
G7-25 | G8 | 17:24:05.62 | −34:07:09.5 | C | ⊃ | Fig. 9 | NGC 6357 region |
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G7-26** | HD 192281 | 20:12:33.12 | +40:16:05.45 | D | ? | − | Special case |
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G7-27* | Vela X-1 | 09:02:06.86 | −40:33:16.9 | E, F | ⊃ | Fig. 5 | HIP 44368, Group 3, HMXB |
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G7-28 | 4U 1907+09 | 19:09:37.9 | +09:49:49 | F | ⊃ | Fig. 10 | HMXB |
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G7-29 | 4U 1700-37 | 17:03:56.77 | −37:50:38.92 | G | ? | − | HMXB |
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G7-30 | J1117-6120 | 11:17:12.93 | −61:20:08.6 | H | ⊃ | Fig. 10 | NGC 3603 region |
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G7-31 | TYC 3159-6-1 | 20:18:40.37 | 41:32:45 | I | ⊃ | − | Cygnus-X region |
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G7-32 | BD −14 5040 | 18:25:38.9 | −14:45:05.74 | J | ⊃ | Fig. 10 | NGC 6611 region |
G7-33* | HD 165319 | 18:05:58.84 | −14:11:52.9 | J | ⊃ | − | NGC 6611 region, HIP 88652, Group 2 |
G7-34 | Star 1 | 18:15:23.97 | −13:19:35.8 | J | ⊃ | Fig. 10 | NGC 6611 region |
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G7-35 | H1 | 15:00:58.55 | −63:16:54.7 | K | † | − | Near: YSO and HH 139 |
G7-36 | H2 | 20:21:18.99 | +34:57:50.96 | L | † | − | Probable YSO |
G7-37 | H3 | 20:34:12.92 | +41:08:15.94 | M | † | − | EGGs (evaporating gaseous globules) |
G7-38** | H4 | 05:46:51.51 | +25:03:48.18 | ⊃? | − | Probable BSC? | |
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G7-39 | SER1 | 08:58:29.4 | −43:25:09 | ⊃ | Fig. 10 | Probably produced by TYC 7688-424-1 | |
G7-40 | SER2 | 10:03:42 | −58:30:28 | ⊃ | Fig. 10 | Not clear | |
G7-41** | SER3 | 10:38:19 | −58:53:22 | ⊃ | Fig. 11 | Probably produced by HD 303197 | |
G7-42** | SER4 | 23:46:37 | +66:46:20 | ⊃ | Fig. 11 | Probably produced by HIP 117265 | |
G7-43 | SER5 | 07:06:33.6 | −11:17:24.5 | ⊃ | Fig. 11 | Probably produced by HIP 34301 | |
G7-44 | SER6 | 01:11:24.3 | +57:33:38 | ⊃ | Fig. 11 | Not clear | |
G7-45 | SER7 | 17:01:20 | −38:12:24.5 | ⊃ | Fig. 11 | Not clear |
Notes. Number: G7 stands for “Group 7” and the number from 01 to 45 is specific of this table. For G7 01 to 34 we looked for bow-shock candidates in WISE images using sources from other works (references in Col. 5). G7 39 to 45 were serendipitously discovered during the catalogue production. Coordinates: for stars that produce the bow shock (whenever possible), or BSC apex coordinates estimated by us (visually), where the star could not be identified. ⊃: BS shape observed in WISE images, ⊃?: BSC to be confirmed, •: emission excess in the region of BS, ?: doubtful cases, detailed in section Special cases, †: not enough resolution to identify bow-shock shape in WISE images. Figure: reference to the figures in the present work. Comments: a relevant comment for each case.
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