All Tables

Table 1: Derived maximum velocities where the blue and red wings reach the continuum. Listed are some forbidden emission lines and some Balmer lines in the FEROS spectrum whose maximum wing velocities could be determined well and which are not blended.
Table 2: Best fit model parameters for the polar (p), intermediate (i), and disk wind (d). The mass fluxes are assumed to be constant within the indicated $\theta$ -ranges and have an error on the order of 20%.
Table 3: Observed and modelled forbidden line luminosities. For the observed values, we took the intensities given in Table 4 and assumed a distance of 2 kpc. The fifth column contains the ratio of observed over modelled line luminosity, and in the sixth column we describe in which part(s) of the wind the line is produced. The classifications of p, i, and d mean polar wind, intermediate wind, and disk, respectively. In the upper part we gathered the lines used to derive the mass fluxes and temperature distributions in each wind zone, while the lines in the lower part have been used to confirm the models and to derive the abundance, especially in the case of N.
Table 4: Emission line intensities relative to H $\beta$ = 100 obtained with B&C spectrograph.