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Table 3
Tangential directions of spiral arms derived from the best-fitted models.
Models\Spiral arms | Near 3 kpc | Scutum | Sagittarius | Carina | Centaurus | Norma | Far 3 kpc | ![]() |
24° | 30.5° | 49.3° | 282° | 310° | 328° | 338° | ||
|
||||||||
Best-fitted models to HII regions, R0 = 8.5 kpc, Θ0 = 220 km s-1. | ||||||||
3-arm model | 22.6 [1.4] | 34.7 [4.2] | 57.5 [8.2] | 285.0 [3.0] | 312.5 [2.5] | 327.4 [0.6] | 1.7 | |
4-arm model | 22.1 [1.9] | 33.6 [3.1] | 55.3 [6.0] | 284.7 [2.7] | 309.8 [0.2] | 324.2 [3.8] | 1.4 | |
PL model | 24.3 [0.3] | 33.3 [2.8] | 51.1 [1.8] | 286.1 [4.1] | 310.2 [0.2] | 326.8 [1.2] | 0.9 | |
|
||||||||
Best-fitted models to all three kinds of spiral tracers. | ||||||||
3-arm model | 22.3 [1.7] | 37.5 [7.0] | 58.7 [9.4] | 283.7 [1.7] | 310.9 [0.9] | 327.4 [0.6] | 2.0 | |
4-arm model | 21.2 [2.8] | 34.9 [4.4] | 54.1 [4.8] | 286.1 [4.1] | 311.9 [1.9] | 326.8 [1.2] | 1.4 | |
PL model | 24.9 [0.9] | 33.6 [3.1] | 50.8 [1.5] | 286.5 [4.5] | 310.1 [0.1] | 326.6 [1.4] | 1.0 | |
|
||||||||
Best-fitted models to HII regions, R0 = 8.3 kpc, Θ0 = 239 km s-1. | ||||||||
3-arm model | 21.9 [2.1] | 35.1 [4.6] | 54.6 [5.3] | 286.1 [4.1] | 312.8 [2.8] | 328.0 [0.0] | 1.5 | |
4-arm model | 22.4 [1.6] | 33.5 [3.0] | 54.7 [5.4] | 285.9 [3.9] | 310.8 [0.8] | 324.1 [3.9] | 1.4 | |
PL model | 23.8 [0.2] | 32.5 [2.0] | 49.7 [0.4] | 288.9 [6.9] | 310.2 [0.2] | 327.3 [0.7] | 1.2 | |
|
||||||||
Best-fitted models to all three kinds of spiral tracers. | ||||||||
3-arm model | 21.6 [2.4] | 36.0 [5.5] | 55.3 [6.0] | 287.0 [5.0] | 312.3 [2.3] | 328.1 [0.1] | 1.7 | |
4-arm model | 22.4 [1.6] | 35.8 [5.3] | 53.9 [4.6] | 287.6 [5.6] | 311.9 [1.9] | 326.3 [1.7] | 1.6 | |
PL model | 22.9 [1.1] | 32.7 [2.2] | 51.7 [2.4] | 288.7 [6.7] | 310.6 [0.6] | 327.9 [0.1] | 1.3 |
Notes. The deviations between the modeled and observed tangential
directions (, see Table 2 for
) are
given in brackets.
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