| Issue |
A&A
Volume 578, June 2015
|
|
|---|---|---|
| Article Number | A81 | |
| Number of page(s) | 14 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201425347 | |
| Published online | 10 June 2015 | |
Online material
Appendix A: Figures
 |
Fig. A.1
Molecule distribution of HCN, CN, H2CO, HCO+, SO, and CS as a function of radius r and z/r (where z is the height over the midplane) for model E. |
| Open with DEXTER | |
 |
Fig. A.2
Distribution of H nuclei volume density (left) and temperature (right) as a function of radius r and z/r (where z is the height over the midplane) in model E. |
| Open with DEXTER | |
 |
Fig. A.3
Top: model A, bottom: model B. Comparison between modeled spectra and those detected by 30 m telescope toward AB Aur disk. In colors we see the synthetic line profile obtain with our model. The blue and magenta lines correspond to the same model with inclination angles for the disk of 27◦ and 40◦ respectively. Vertical dash line indicate the Vlsr = 5.9 km s-1 (Duvert et al. 1986). |
| Open with DEXTER | |
 |
Fig. A.4
Top: model C; bottom: model D. |
| Open with DEXTER | |
© ESO, 2015
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