Up: Kinematics of the local
Line widths are measured on the observed profile at two standard
levels corresponding to 20% and 50% of the maximum intensity
of the line. The results listed in Table 7 (Cols. 7 and 9)
have been corrected to the optical velocity scale. According to
Fouqué et al. (1990), the mean measurement error is
equal to
and
for the 20% and 50% widths, respectively.
We give in column 11 the derived
value of the logarithm of the maximum of circular velocity
.It has been calculated as follows. The widths W20 and W50
are first corrected for resolution effect:

for l= 20 and l=50 (Bottinelli et al. 1990),
and further corrected for internal velocity dispersion:

where
, assuming an isotropic distribution
of the non-circular motions
= 12 km s-1 and a nearly
gaussian velocity distribution (k(20)=1.96 and k(50)=1.13;
Fouqué
et al.1990).
Corrected W20 and W50 are finally used to calculate
:

Where the inclination incl is derived from:

R25 is the axis ratio and
= 0.43 + 0.053T
for type T= 1 to 7 and
=0.38 for T=8.
The actual uncertainty on
has been calculated according
to Bottinelli et al. 1983.
94% of our observations have a signal to noise ratio S/N greater
than 3; 62% have a signal to noise ratio greater than 5.
Figure 3 shows the observed line widths as a function of S/N.
For information, the above corrections for resolution effect and
non-circular motions represent on average about 18%
and 11% of the observed line width, for the 20% and 50% level
respectively. They lead to a correction of
3.3% on average on
.
 |
Figure 3:
observed line width, a) and b) , as a function of
signal to noise ratio S/N |
Up: Kinematics of the local
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