Research Article
The Dark Matter Halo Density Profile, Spiral Arm Morphology, and Supermassive Black Hole Mass of M33
Table 1
M33 Observational data. The Hubble type is from de Vaucouleurs et al. [
17]. The distance in kpc is taken from Magrini et al. [
21].
| Parameter | Measurement |
| Hubble type | SA(s)cd | Distance (kpc) | 840 | Position angle of major axis (°) | 23 | Bulge effective radius, (arcmin) | 1.60 ± 0.11 | Bulge effective radius, (kpc) | 0.39 ± 0.03 | Bulge surface brightness at the effective radius, (3.6 μm-mag arcsec−2) | 19.57 ± 0.98 | Bulge Sérsic index, | 1.0 | Disk central surface brightness, (3.6 μm-mag arcsec−2) | 18.08 ± 1.02 | Disk scalelength, (arcmin) | 6.95 ± 0.49 | Disk scalelength, (kpc) | 1.70 ± 0.12 | Disk luminosity, | (3.16 ± 0.30) × 109 | Bulge-to-disk ratio, | 0.03 |
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