![]() |
Figure 1: A schematic illustration of the geometry of a narrow spiral density stream showing that an observer sees a narrow absorption feature corresponding to the radial velocity of the stream material in front of the star at any moment (in the point-star approximation). |
Open with DEXTER |
![]() |
Figure 2:
Comparison of approximate best fit ![]() ![]() ![]() ![]() ![]() ![]() |
Open with DEXTER |
![]() |
Figure 3:
Obtaining the narrow-stream DAC dynamic
spectrum
![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() |
Open with DEXTER |
![]() |
Figure 4:
Solution of
the narrow-stream velocity inversion problem. The upper curve is an
apparent Doppler shift law
![]() ![]() ![]() |
Open with DEXTER |
![]() |
Figure 5:
Ratio of apparent accelerations of a
wide stream DAC peak (a*(w)) to a narrow stream DAC (
![]() ![]() |
Open with DEXTER |
![]() |
Figure 8:
[![]() ![]() |
Open with DEXTER |
![]() |
Figure 11:
[![]() ![]() |
Open with DEXTER |
![]() |
Figure 14:
[![]() ![]() |
Open with DEXTER |
![]() |
Figure 17:
[![]() ![]() |
Open with DEXTER |
![]() |
Figure 18:
Inferred wind rotation law, W(x) for the dynamical spectrum
shown in the left panel of Fig. 6a, that is, for a pure
![]() |
Open with DEXTER |
![]() |
Figure 6:
[
![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() |
Open with DEXTER |
![]() |
Figure 7:
[
![]() ![]() |
Open with DEXTER |
![]() |
Figure 9:
[
![]() |
Open with DEXTER |
![]() |
Figure 10:
[
![]() ![]() |
Open with DEXTER |
![]() |
Figure 12:
[
![]() |
Open with DEXTER |
![]() |
Figure 13:
[
![]() ![]() |
Open with DEXTER |
![]() |
Figure 15:
[
![]() ![]() ![]() ![]() |
Open with DEXTER |
![]() |
Figure 16:
[
![]() ![]() |
Open with DEXTER |