| Issue |
A&A
Volume 532, August 2011
|
|
|---|---|---|
| Article Number | A149 | |
| Number of page(s) | 19 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201116649 | |
| Published online | 09 August 2011 | |
Online material
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Fig. 9
As in Fig. 7, model calculations for the oblate ellipsoid e = 0.7 with equatorial distribution, where the velocity in the equatorial region is twice that in the polar axis. |
| Open with DEXTER | |
 |
Fig. 10
As in Fig. 7, model calculations for the oblate ellipsoid (e = 0.9) with equatorial distribution,where the velocity in the equatorial region is four times higher than that in the polar axis. |
| Open with DEXTER | |
 |
Fig. 11
As in Fig. 7, model calculations for the prolate ellipsoid (e = 0.7) with equatorial distribution, where the velocity in the polar axis is twice than that in the equatorial plane. |
| Open with DEXTER | |
 |
Fig. 12
As in Fig. 7, model calculations for the prolate ellipsoid (e = 0.9) with equatorial distribution, where the velocity in the polar axis is four times higher than that in the equatorial plane. |
| Open with DEXTER | |
 |
Fig. 13
As in Fig. 8, model calculations for the oblate ellipsoid (e = 0.7) with biconical distribution, where the outflow velocity increases towards the equatorial plane. |
| Open with DEXTER | |
 |
Fig. 14
As in Fig. 8, model calculations for the oblate ellipsoid (e = 0.9) with biconical distribution, where the outflow velocity increases towards the equatorial plane. |
| Open with DEXTER | |
 |
Fig. 15
As in Fig. 8, model calculations for the prolate ellipsoid (e = 0.7) with biconical distribution, where the outflow velocity increases towards the polar region. |
| Open with DEXTER | |
 |
Fig. 16
As in Fig. 8, model calculations for the prolate ellipsoid (e = 0.9) with biconical distribution, where the outflow velocity increases towards the polar region. |
| Open with DEXTER | |
© ESO, 2011
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