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Table 3.

Sets of parameters obtained from χ2-minimization to fit the observation profiles with the analytical model.

# XCO δ Q γ0 ξ (1) (2) Qmin(3)


DISK (4) NW (5)
1 (a) 6.6 1.7 0.17 10.6 19.5 1.26 3.3 1.0 1.0 1.3 5.6 3.7 1.0 0.9
(b) ×2 13.5 0.64 4.7 0.8 1.4 2.4

2 (a) 5.7 1.5 0.10 ×2 8.7 18.0 1.20 3.1 0.9 1.1 1.1 3.2 0.8 0.8 1.6
(b) ×2 12.0 0.58 3.7 1.1 1.7 1.0

3 (a) 4.8 1.6 0.11 ×2 10.0 19.8 1.23 3.0 0.9 1.0 1.0 4.1 0.9 1.1 2.1
(b) ×2 12.0 0.50 2.6 1.1 0.8 0.8

4 (a) 11.1 1.6 0.13 ×2 9.4 18.8 1.25 3.1 1.0 1.1 1.0 8.0 1.0 0.9 6.0
(b) ×2 11.1 0.42 4.8 3.2 0.8 0.8

5 (a) 5.7 1.8 0.17 ×2 ×2 11.2 20.5 1.28 2.9 0.9 1.1 0.9 7.9 0.8 0.9 6.2
(b) ×2 14.1 0.57 4.9 2.8 0.8 1.3

6 (a) 10.2 1.9 0.22 ×2 ×2 12.1 20.1 1.29 4.0 1.5 1.1 1.3 12.9 0.8 0.8 11.2
(b) ×2 14.2 0.44 7.2 5.5 0.9 0.8

7 (a) 11.1 1.5 0.13 ×2 ×2 9.1 18.0 1.30 3.8 1.5 1.1 1.1 11.9 1.1 1.6 9.3
(b) ×2 10.7 0.40 6.7 4.4 0.8 1.4

Notes.

(1)

Mean velocity dispersion in the unperturbed disk.

(2)

Maximum velocity dispersion reached in the high H I surface density region.

(3)

Minimum Toomre Q reached in the high H I surface density region.

(4)

χ2 obtained for the southeastern unperturbed disk.

(5)

χ2 obtained for the northwestern perturbed disk. The bold characters correspond to the models with the lowest total χ2 for a galactic conversion factor and a modified conversion factor .

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