Comparison of synthetic maps from truncated jet-formation models with YSO jet observations - II. The effect of varying inclinations

Free Access

Issue		A&A Volume 538, February 2012


Article Number		A116
Number of page(s)		14
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201117948
Published online		13 February 2012

Online material

Appendix A: Extracted line widths for all models and runs

Here we present the extracted line widths derived from synthetic [OI] λ6300 images for all models, runs, and inclinations for the sake of completeness.

	Fig. A.1 Jet widths in AU derived from synthetic [OI] images as a function of distance from the source in model ADO and for runs (500, 600, 0.2), (500, 600, 0.5), (500, 1000, 0.5), (500, 1000, 0.8). Overlaid are the data points of Fig. 1.
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	Fig. A.2 Same as Fig. A.1, but in model SC1a.
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	Fig. A.3 Same as Fig. A.1, but in model SC1b.
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	Fig. A.4 Same as Fig. A.1, but in model SC1c.
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	Fig. A.5 Same as Fig. A.1, but in model SC1d.
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	Fig. A.6 Same as Fig. A.1, but in model SC1e.
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	Fig. A.7 Same as Fig. A.1, but in model SC1f.
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	Fig. A.8 Same as Fig. A.1, but in model SC1g.
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Appendix B: Velocities of the jet derived from the synthetic position-velocity diagrams

Table B.1

Velocities of the jet derived from the synthetic position-velocity diagrams for model ADO.

Table B.2

Same as Table B.1, but for model SC1a.

Table B.3

Same as Table B.1, but for model SC1b.

Table B.4

Same as Table B.1, but for model SC1c.

Table B.5

Same as Table B.1, but for model SC1d.

© ESO, 2012

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