Table 6 : part 4
OHP preprint 132
Table:
Fitting profile analysis results. Col. 1 gives the
name of the
object, col. 2 the adopted redshift, cols. 4 and 9 the velocities for each
set of components measured on the blue and red spectra, respectively, and
de-redshifted using the redshift given in col. 2; cols. 5 and 10 the
corresponding FWHM, cols. 6, 11 and 12 the intensity ratios
5007/H,
6583/H and 6300/H respectively, and cols. 7 and 13 the
fraction of the emission
flux (respectively ) in each component with respect to the
total flux of the line in each object. A ``T'' in col. 3
(or 8) indicates that the blue (or red) spectrum has been corrected for
starlight using a suitable fraction of a template (in the blue, we have used
the elliptical galaxy NGC 5982 and in the red, the elliptical galaxy NGC
4365;
NGC 821 was used as a template for the objects observed in October and
November
1997); in the same columns, an ``A'' indicates that a (or )
absorption component was added to the model. In col. 14 we give the
velocity difference between the blue and red systems, and in col. 15 the
spectroscopic classification of each component in
the model; Gaussian profiles were
used throughout, except when indicated by ``lz'' (Lorentzian profile)
.
Values in parenthesis have been fixed.
Name |
z |
Stellar |
|
FWHM |
5007 |
|
Stellar |
|
FWHM |
6583 |
6300 |
|
|
Class. |
|
|
corr. |
(kms-1) |
(kms-1) |
|
(%) |
corr. |
(kms-1) |
(kms-1) |
|
|
(%) |
(kms-1) |
|
Mark 938 |
0.019 |
A |
111 |
240 |
1.18 |
91 |
T |
173 |
270 |
0.71 |
0.07 |
89 |
-62 |
Hii |
|
|
|
(-79) |
890 |
(10) |
9 |
|
-11 |
648 |
6.78 |
< 0.3 |
11 |
-68 |
Sey2 |
Mark 957 |
0.0732 |
|
-402 |
710 |
9.00 |
8 |
|
-201 |
726 |
1.35 |
< 0.3 |
18 |
-201 |
Sey2 |
|
|
|
-43 |
200 |
0.15 |
92 |
|
3 |
192 |
0.35 |
< 0.02 |
82 |
-46 |
Hii |
IRAS 01346-0924 |
0.070 |
|
114 |
178 |
2.13 |
38 |
|
165 |
148 |
0.70 |
< 0.04 |
23 |
-51 |
Hii |
|
|
|
-83 |
< 80 |
0.83 |
39 |
|
-33 |
219 |
0.46 |
0.07 |
37 |
-50 |
Hii |
|
|
|
-224 |
1069 |
(10) |
23 |
|
- |
- |
- |
- |
- |
- |
Sey2 |
|
|
|
- |
- |
- |
- |
|
219 |
2640 |
- |
- |
40 |
- |
Sey1 |
Mark 1066 |
0.0122 |
|
-116 |
348 |
12.38 |
11 |
|
-51 |
270 |
0.77 |
0.07 |
35 |
-65 |
Sey2 |
|
|
|
30 |
220 |
1.54 |
66 |
|
54 |
205 |
0.89 |
0.08 |
39 |
-24 |
Hii |
|
|
|
-262 |
875 |
5.76 |
23 |
|
-165 |
(875) |
1.49 |
0.15 |
26 |
-97 |
Sey2 |
IRAS 03355+0104 |
0.0398 |
|
-1 |
364 |
13.69 |
100 |
|
12 |
354 |
0.49 |
0.12 |
66 |
-13 |
Sey2 |
|
|
|
- |
- |
- |
- |
|
264 |
1930 |
- |
- |
34 |
- |
Sey1 |
IRAS 04210+0400 |
0.0462 |
|
14 |
178 |
13.30 |
41 |
|
63 |
219 |
0.40 |
0.17 |
47 |
-49 |
Sey2 |
|
|
|
0 |
541 |
13.03 |
59 |
|
41 |
615 |
0.34 |
0.06 |
53 |
-41 |
Sey2 |
IRAS 04507+0358 |
0.0296 |
|
-28 |
240 |
11.00 |
82 |
|
14 |
282 |
0.47 |
0.09 |
64 |
-42 |
Sey2 |
|
|
|
-146 |
603 |
14.57 |
18 |
|
- |
- |
- |
- |
- |
- |
Sey2 |
|
|
|
- |
- |
- |
- |
|
-88 |
1254lz |
- |
- |
36 |
- |
Sey1 |
VII Zw 73 |
0.0405 |
|
0 |
307 |
(15) |
28 |
|
17 |
272 |
0.80 |
0.10 |
37 |
-17 |
Sey2 |
|
|
|
-186 |
794 |
(15) |
12 |
|
-171 |
685 |
0.52 |
0.22 |
16 |
15 |
Sey2 |
|
|
|
3 |
151 |
1.28 |
60 |
|
14 |
111 |
0.48 |
0.02 |
47 |
-11 |
Hii |
Mark 622 |
0.0233 |
T, A |
6 |
178 |
(0.1) |
59 |
T |
12 |
205 |
0.79 |
0.06 |
49 |
-6 |
Hii |
|
|
|
-58 |
1172 |
(10) |
41 |
|
-22 |
748 |
1.44 |
< 0.5 |
51 |
-36 |
Sey2 |
3C 198.0 |
0.081 |
|
- |
- |
- |
- |
|
125 |
294 |
0.28 |
0.05 |
100 |
- |
? |
KUG 0825+248 |
0.083 |
|
108 |
< 80 |
0.62 |
100 |
|
135 |
95 |
0.29 |
0.02 |
100 |
-27 |
Hii |
IRAS 09111-1007E |
0.055 |
|
-113 |
< 80 |
(0.1) |
16 |
|
-230 |
95 |
0.55 |
< 0.09 |
12 |
117 |
Hii |
|
|
|
(-76) |
259 |
(0.1) |
53 |
|
-41 |
257 |
0.86 |
< 0.05 |
40 |
-35 |
Hii |
|
|
|
-113 |
430 |
(10) |
31 |
|
-96 |
626 |
0.95 |
0.12 |
48 |
-17 |
Sey2 |
Zw 238.066 |
0.034 |
T, A |
95 |
220 |
0.60 |
54 |
A |
149 |
< 80 |
0.69 |
< 0.05 |
14 |
-54 |
Hii |
|
|
|
-134 |
154 |
1.33 |
37 |
|
-71 |
307 |
0.79 |
0.05 |
78 |
-63 |
Hii |
|
|
|
-295 |
935 |
(10) |
9 |
|
-529 |
1130 |
3.75 |
< 0.6 |
8 |
234 |
Sey2 |