Parameters of the exciting stars and H ii regions from the literature used in the present study.
| H ii region . | Exciting star . | Te . |
|---|---|---|
| . | . | (K) . |
| S254 | O9.0V1, O9.0V3 | – |
| S255 | B0.0V1, B0.0V3 | 82004, 8833 ± 1707 |
| S256 | B2.5V2, B0.9V3 | – |
| S257 | B0.5V1 | 6900–79005, 7970 ± 2606 |
| S258 | B3V2, B1.5V3 | – |
| H ii region . | Exciting star . | Te . |
|---|---|---|
| . | . | (K) . |
| S254 | O9.0V1, O9.0V3 | – |
| S255 | B0.0V1, B0.0V3 | 82004, 8833 ± 1707 |
| S256 | B2.5V2, B0.9V3 | – |
| S257 | B0.5V1 | 6900–79005, 7970 ± 2606 |
| S258 | B3V2, B1.5V3 | – |
References:1 Moffat, Fitzgerald & Jackson (1979), 2 Russeil, Adami & Georgelin (2007), 3 Chavarría et al. (2008), 4 Fernández-Martín et al. (2017), 5 Méndez-Delgado et al. (2022), 6 Esteban & García-Rojas (2018), 7G192.638-00.008 in Wenger et al. (2019).
Parameters of the exciting stars and H ii regions from the literature used in the present study.
| H ii region . | Exciting star . | Te . |
|---|---|---|
| . | . | (K) . |
| S254 | O9.0V1, O9.0V3 | – |
| S255 | B0.0V1, B0.0V3 | 82004, 8833 ± 1707 |
| S256 | B2.5V2, B0.9V3 | – |
| S257 | B0.5V1 | 6900–79005, 7970 ± 2606 |
| S258 | B3V2, B1.5V3 | – |
| H ii region . | Exciting star . | Te . |
|---|---|---|
| . | . | (K) . |
| S254 | O9.0V1, O9.0V3 | – |
| S255 | B0.0V1, B0.0V3 | 82004, 8833 ± 1707 |
| S256 | B2.5V2, B0.9V3 | – |
| S257 | B0.5V1 | 6900–79005, 7970 ± 2606 |
| S258 | B3V2, B1.5V3 | – |
References:1 Moffat, Fitzgerald & Jackson (1979), 2 Russeil, Adami & Georgelin (2007), 3 Chavarría et al. (2008), 4 Fernández-Martín et al. (2017), 5 Méndez-Delgado et al. (2022), 6 Esteban & García-Rojas (2018), 7G192.638-00.008 in Wenger et al. (2019).
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