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Table 3.
Optically detected emission-line objects in NGC 185 galaxy.
| RA | Dec | Hα flux (a) | [S II] flux | D(b) | Cross- | ||
|---|---|---|---|---|---|---|---|
| ID | (h:m:s) | (d:m:s) | [10−15 | [10−15 | [pc] | ID (c) | Comment |
| J2000 | J2000 | erg cm−2 s−1] | erg cm−2 s−1] | ||||
| VIEM 1 | 00:38:47:9 | 48:19:32 | 0.8 ± 0.1 | – | < 6 | 5-PN5 | PN |
| VIEM 2 | 00:38:53.1 | 48:20:08 | 8.9 ± 0.1 | – | < 6 | 1-PN1 | PN |
| VIEM 3 | 00:38:54.4 | 48:20:01 | 0.7 ± 0.1 | – | < 6 | 10-PN8 | PN |
| VIEM 4 | 00:38:56.4 | 48:19:21 | 14.9 ± 0.1 | – | < 6 | 4-PN4 | PN |
| VIEM 5 | 00:38:57.3 | 48:20:10 | 7.0 ± 0.1 | – | < 6 | 2-PN2 | PN |
| VIEM 6 | 00:38:57.3 | 48:20:35 | 0.2 ± 0.1 | – | 6 | 8-PN7 | Contribution of shocks |
| VIEM 7 | 00:38:57.5 | 48:20:16 | 2.0 ± 0.1 | 1.0 ± 0.1 | < 6 (d) | 9-SNR1 | H II region |
| VIEM 8 | 00:38:58.2 | 48:20:09 | 28.7 ± 5.0 | 35.8 ± 5.0 | 45 | SNR | |
| VIEM 9 | 00:38:59.0 | 48:20:17 | 6.0 ± 5.6 | 2.4 ± 5.6 | 50 | SNR | |
| VIEM 10 | 00:39:00.2 | 48:19:47 | 3.3 ± 0.1 | – | < 6 | 3-PN3 | PN |
| VIEM 11 | 00:39:00.3 | 48:19:27 | 0.6 ± 0.1 | – | < 6 | 13-StSy | Symbiotic star |
Notes.
(a)
Flux has been corrected for [N II] emission, as described in the text, and for Galactic extinction, assuming that A(Hα) = 0.6AB; AB = 0.667 (Schlafly & Finkbeiner 2011).
(c)
IDs from Gonçalves et al. (2012).
(d)
Gonçalves et al. (2012) give estimate of 2 pc.
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