Astron. Astrophys. 329, 792-798 (1998)
4. Extrapolation method for the contribution of the first three angular momenta to the total profile
Feautrier et al. (1976) and Feautrier and Tran Minh (1977) used two
methods to determine the contribution of the first angular momenta
( , 1 and 2), excluded by the exact resonance
approximation. The first, based on the program of Seaton and Wilson
(1972), consisted of solving the coupled integro-differential
equation; and the second leaned on a semi-empirical approach. A rapid
and accurate method is still needed for the calculation of this
contribution. The present extrapolation procedure consists of
continuing the curve of the contribution of the angular momenta to the
total profile ( ) such as to find the
contributions relative to , 1 and 2 with the
minimum error. A good choice for this extrapolation is obtained by
completing the original curve by a straight line connecting the point
to the point (Fig.1).
The contribution of the first three angular momenta is thus found to
be:
![[FIGURE]](img74.gif) |
Fig. 1. Extrapolation of the contribution of the first three angular momenta to the total profile for Å . Data from the exact quantum calculations are presented in Feautrier et al. (1976)
|
![[EQUATION]](img76.gif)
while the sum of errors due to extrapolation of the three points is
about . On the other hand, since there is a
balancing of the 's in the sum around the
extrapolation line, the actual error is about .
Hence, the total profile, normalized to in the
dipole approximation and taking into account each of the
's contribution is:
![[EQUATION]](img81.gif)
Numerically, the error in the so-determined total profile is found
to vary from about less than in the near line
wings to about less than the far wings.
Further, it decreases with increasing temperature. The present
extrapolation procedure, which has been checked to provide results in
good agreement with the semi-empirical method of Feautrier and Tran
Minh (1977) is advantageous for its rapidity and its simplicity.
© European Southern Observatory (ESO) 1998
Online publication: December 8, 1997
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