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Source | Radio | Infrared | RA | Dec | Countsa | Median | Temperature | Absorption | Luminosity | Radio | Spectral | Infrared |
ID | ID | ID | energyb | kT (keV) | 1022 cm-2 |
![]() |
flux (mJy) | index | magc | |||
X1 | IRS 6b | 22:56:22.2 | +62:02:00.5 | 137 | 2.3 | 2.0-3.0 | 1.4-2.2 | 30.7-30.9 | - | 8.4 | ||
X2 | IRS 6d | 22:56:20.9 | +62:02:04.0 | 44 | 4.2 | 2.0e | 10-18 | 30.9-31.1 | - | 11.1 | ||
1.0e | 20 - 32 | 32.0-32.3 | ||||||||||
X3 | ?d | 22:56:17.4 | +62:01:58.6 | 36 | 4.3 | 2.0e | 10-18 | 30.9-31.1 | - | |||
1.0e | 17-26 | 31.8-32.1 | ||||||||||
X4 | GPFW 2 | 22:56:20.2 | +62:01:41.4 | 64 | 3.9 | 0.9-1.7 | 11-32 | 31.2-32.3 | - | 15.6 | ||
X5 | 9 | 22:56:18.6 | +62:01:47.8 | 60 | 4.1 | 0.7-1.3 | 20-38 | 31.8-33.4 | 3.0 | -0.2 | ||
X6 | 22:56:18.1 | +62:01:43.2 | 50 | 5.5 | 2.0e | 32-50 | 31.5-31.8 | - | ||||
1.0e | 61-83 | 33.1-33.4 | ||||||||||
X7 | 3c | 22:56:18.0 | +62:01:46.0 | 60 | 6.4 | 2.0e | 62-106 | 32.1-32.5 | 3.7 | 0.4 | ||
(1.0e | 127-175 | 34.0-34.5)f | ||||||||||
1a | 22:56:16.2 | +62:01:37.8 | 2 | - | <29.8 (30.5) | 2.2 | -0.6 | |||||
1b | 22:56:16.6 | +62:01:42.6 | 2 | - | <29.8 (30.5) | 2.9 | -0.3 | |||||
2 | 22:56:19.0 | +62:01:49.4 | <4 | - | <30.0 (30.7) | 7.5 | 0.7 | |||||
3a | GPFW 1a? | 22:56:17.1 | +62:01:43.9 | 1 | - | <29.6 (30.3) | 0.2 | - | 14.7 | |||
3b | 22:56:17.7 | +62:01:45.0 | 6 | 4.6 | - | 29.9 (30.6) | 5.0 | 0.0 | ||||
3d | 22:56:18.2 | +62:01:46.0 | 3 | - | <29.9 (30.6) | 7.7 | 0.3 | |||||
4 | GPFW 3 | 22:56:18.5 | +62:01:56.0 | 1 | - | <29.6 (30.3) | 4.4 | -0.2 | 12.6 | |||
5 | 22:56:19.7 | +62:01:59.5 | 1 | - | <29.6 (30.3) | 1.3 | -0.5 | |||||
6 | 22:56:20.2 | +62:02:03.0 | 0 | - | <29.2 (29.9) | 3.8 | -0.3 | |||||
7a | 22:56:20.2 | +62:01:39.9 | 2 | - | <29.8 (30.5) | 9.6 | -0.1 | |||||
7b | 22:56:20.8 | +62:01:39.6 | 1 | - | <29.6 (30.3) | 2.8 | -0.4 | |||||
7c | 22:56:21.4 | +62:01:37.4 | 0 | - | <29.2 (29.9) | 3.8 | -0.4 | |||||
7dg | 22:56:21.9 | +62:01:36.5 | 1 | - | <29.7 (30.4) | 2.4 | - | |||||
8 | 22:56:17.7 | +62:01:47.0 | 9 | 6.2 | - | 30.1 (30.8) | <0.12 | - | ||||
IRS 6c | 22:56:17.5 | +62:01:51.1 | 1 | - | <29.6 (30.3) | - | 8.5h |
a Including a background of 1.3 cts; b in keV; c K-band; d visible in the Goetz et al. (1998) IR-images; e fixed; f this value is unlikely high for a stellar source, see Sect. 3.2.2; g data from Hughes & Wouterloot (1984); h L-band.
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