Free Access
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

thumbnail 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.

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thumbnail 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.

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thumbnail 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).

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thumbnail Fig. A.4

Top: model C; bottom: model D.

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© ESO, 2015

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