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Table 2
Structural parameters of the stellar and dust components from different studies.
| Reference | Band | i | hR, ∗ | hz, ∗ | h R,d | h z,d | r e,b |
|
| (deg) | (kpc) | (kpc) | (kpc) | (kpc) | (kpc) | |||
|
|
||||||||
| (1) | B | 89.6 ± 0.2 | 11.34 ± 0.17 | 0.72 ± 0.02 | 14.85 ± 0.50 | 0.45 ± 0.02 | 3.28 ± 0.25 | 0.40 ± 0.01 |
| (1) | V | 89.6 ± 0.2 | 8.73 ± 0.17 | 0.69 ± 0.02 | 13.68 ± 0.33 | 0.38 ± 0.02 | 2.06 ± 0.13 | 0.30 ± 0.01 |
| (1) | I | 89.6 ± 0.2 | 8.45 ± 0.17 | 0.72 ± 0.02 | 14.10 ± 0.33 | 0.35 ± 0.02 | 2.63 ± 0.13 | 0.22 ± 0.01 |
| (1) | J | 89.7 ± 0.2 | 8.30 ± 0.50 | 0.74 ± 0.17 | 13.51 ± 1.00 | 0.33 ± 0.12 | 3.29 ± 0.17 | 0.06 ± 0.02 |
| (1) | K | 89.6 ± 0.2 | 8.43 ± 0.17 | 0.75 ± 0.03 | 13.38 ± 0.50 | 0.37 ± 0.05 | 3.34 ± 0.40 | 0.02 ± 0.01 |
| (2) | I | – | 17.3 ± 0.9 | 0.9 ± 0.1 | – | – | 1.79 ± 0.05 | – |
| (3) | K s | – | 6.36 ± 0.57 | 0.46 | – | – | – | – |
Notes. The sizes have been rescaled to the distance presented in Table 1. The models from (2) and (3) assume a perfect edge-on disc orientation.
Reference. (1) Xilouris et al. (1999); (2) Kregel et al. (2002); (3) Bizyaev & Mitronova (2009).
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