Kinematic modeling of disk galaxies - III. The warped “Spindle” NGC 2685

Table C.1:

Radially dependent best-fit parameters.
$r_{\rm p}$	$r_{\rm t}$	$\Delta~r_{\rm t}$	$I_{\rm tot,f}$	$\Delta~I_{\rm tot,f}$	$N_{\rm {H~{\sc i}}}$	$\Delta~N_{\rm {H~{\sc i}}}$	$\sigma$	$\Delta~\sigma$	$V_{\rm rot}$	$\Delta~V_{\rm rot}$	i	$\Delta~i$	pa	$\Delta~pa$	$n_{\rm W}$	$\Delta~n_{\rm W}$	$n_{\rm N}$	$\Delta~n_{\rm N}$	$n_{\rm LOS}$	$\Delta~n_{\rm LOS}$
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)	(14)	(15)	(16)	(17)	(18)	(19)	(20)	(21)
0	0.00	0.00	0.0	2.0	0.0	2.5	0.0	0.2	0.0	0.0
12	0.88	0.22	0.0	2.0	0.0	2.5	0.0	0.2	154.2	79.0	35.3	18.7	245.0	68.7	-0.524	0.379	0.244	0.639	0.816	0.189
24	1.77	0.44	8.8	20.8	10.9	25.9	0.9	2.1	134.9	13.1	65.4	11.7	217.7	10.5	-0.556	0.142	0.720	0.122	0.416	0.186
36	2.65	0.66	72.4	7.3	90.4	9.1	7.2	0.7	131.2	5.6	69.7	4.0	204.7	4.0	-0.392	0.060	0.852	0.035	0.348	0.065
48	3.54	0.87	57.2	12.1	71.5	15.1	5.7	1.2	144.6	10.0	54.4	4.9	197.9	5.9	-0.249	0.081	0.774	0.054	0.582	0.070
60	4.42	1.09	33.5	11.8	41.9	14.7	3.4	1.2	163.9	30.5	47.8	7.6	160.0	8.9	0.253	0.112	0.696	0.093	0.672	0.099
72	5.31	1.31	39.0	11.5	48.7	14.3	3.9	1.1	146.1	18.2	41.5	8.3	161.1	10.9	0.215	0.125	0.627	0.111	0.749	0.096
84	6.19	1.53	15.9	11.2	19.8	14.0	1.6	1.1	183.1	41.9	31.0	11.3	147.4	4.1	0.277	0.096	0.434	0.144	0.857	0.101
96	7.08	1.75	22.0	9.9	27.4	12.4	2.2	1.0	184.0	20.7	33.6	13.6	120.0	12.5	0.479	0.182	0.276	0.144	0.833	0.132
108	7.96	1.97	14.0	8.6	17.5	10.8	1.4	0.9	141.5	6.4	60.6	4.0	132.9	6.4	0.638	0.071	0.593	0.075	0.490	0.061
120	8.85	2.19	21.9	3.9	27.4	4.9	2.2	0.4	160.0	8.2	59.5	4.0	126.1	4.0	0.696	0.046	0.508	0.053	0.507	0.060
140	10.32	2.55	16.8	2.0	21.0	2.5	1.7	0.2	152.2	11.6	67.3	4.0	122.6	4.0	0.777	0.041	0.497	0.056	0.385	0.064
160	11.80	2.91	17.5	2.0	21.8	2.5	1.7	0.2	151.0	8.2	70.0	4.0	125.5	4.0	0.765	0.043	0.545	0.055	0.342	0.066
180	13.27	3.28	15.2	2.0	18.9	2.5	1.5	0.2	156.4	8.2	69.1	4.2	126.7	4.0	0.749	0.044	0.558	0.055	0.358	0.068
200	14.75	3.64	5.0	2.0	6.2	2.5	0.5	0.2	152.1	8.2	64.5	7.0	125.8	4.0	0.732	0.057	0.527	0.060	0.431	0.111
240	17.69	4.37	2.4	2.0	3.0	2.5	0.2	0.2	147.5	8.2	63.6	4.0	124.5	4.0	0.738	0.044	0.507	0.054	0.445	0.063
280	20.64	5.10	2.0	2.0	2.5	2.5	0.2	0.2	137.5	8.2	62.5	4.0	121.3	4.2	0.758	0.044	0.460	0.059	0.462	0.062
320	23.59	5.83	0.5	2.0	0.6	2.5	0.0	0.2	143.9	15.0	64.8	4.3	123.2	13.7	0.757	0.122	0.496	0.182	0.425	0.068
360	26.54	6.56	0.8	2.0	1.0	2.5	0.1	0.2	139.6	15.0	66.7	4.0	121.9	7.1	0.780	0.065	0.485	0.098	0.396	0.064
400	29.49	7.29	0.2	2.0	0.2	2.5	0.0	0.2	146.7	15.0	66.9	8.4	119.5	10.0	0.801	0.093	0.454	0.143	0.392	0.134
420	30.96	7.65	0.9	2.0	1.2	2.5	0.1	0.2	168.8	15.0	67.4	10.6	119.0	10.0	0.807	0.100	0.448	0.145	0.384	0.171

(1) Radius ( $~\hbox{$^{\prime\prime}$ }$ ); (2) radius ( $\rm kpc$ , according to Table 1); (3) error of $r_{\rm t}$ ( $\rm kpc$ ); (4) face-on surface brightness ( ${\rm Jy}~{\rm km}~{\rm s}^{-1}$ ); (5) error of $I_{\rm tot,f}$ ( ${\rm Jy}~{\rm km}~{\rm s}^{-1}$ ); (6) face-on H I column-density ( $10^{19}~{\rm atoms}~{\rm cm}^{-2}$ ); (7) error of $N_{\rm {H~{\sc i}}}$ ( $10^{19}~{\rm atoms}~{\rm cm}^{-2}$ ); (8) face-on surface density ( ${\rm M}_{\odot}~{\rm pc}^{-2}$ ); (9) error of $\sigma$ ( ${\rm M}_{\odot}~{\rm pc}^{-2}$ ); (10) rotation velocity ( $\rm km~{\rm s}^{-1}$ ); (11) error of $V_{\rm rot}$ ( $\rm km~{\rm s}^{-1}$ ); (12) inclination ( $~\hbox{$^\circ$ }$ ); (13) error of i ( $~\hbox{$^\circ$ }$ ); (14) position angle ( $~\hbox{$^\circ$ }$ ); (15) error of pa ( $~\hbox{$^\circ$ }$ ); (16) inclination ( $~\hbox{$^\circ$ }$ ); (17)-(23) are Cartesian components of the spin normal vector ${\vec n}$ of the ring and their errors; (17) spin normal vector component towards W (natural units); (18) Error of $n_{\rm W}$ (natural units); (19) spin normal vector component towards N (natural units); (20) error of $n_{\rm N}$ (natural units); (21) spin normal vector component towards observer (natural units); (22) error of $n_{\rm LOS}$ (natural units).

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