These models are equivalent to the disc-wind magnetospher hybrid model with Mdot_acc=1x10^-8 Msun/yr & Mdot_wind=1x10^-9 Msun/yr in the paper EXCEPT a smaller source displacement distance (d = 5Rstar) is used in these models where Rstar is the stellar radius. In the paper, d=22Rstar was used. With d=5Rstar, the wind launching (magneto-centrifugal) condition of of Blandford & Payne (1982, MNRAS, 199, 883) is satisfied everywhere in the disc wind launching zones. The absorption feature in the profiles are weaken in i=55 deg models (see below), but the overall profile morphology is very similar to that of the models computed with d=22Rstar.
Models are computed at inclination angles of 10, 55 and 80 degrees. At each inclination angle, the profiles are computed with combinations of a wind temperatures (7000K, 8000K, 9000K) and a wind accerelation parameter beta (0.2, 0.5, 1.0, 2.0).
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Inclination angle = 10 degrees
Inclination angle = 55 degrees
Inclination angle = 80 degrees