Volume 538, February 2012
|Number of page(s)||14|
|Section||Interstellar and circumstellar matter|
|Published online||13 February 2012|
Here we present the extracted line widths derived from synthetic [OI] λ6300 images for all models, runs, and inclinations for the sake of completeness.
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.
|Open with DEXTER|
Velocities of the jet derived from the synthetic position-velocity diagrams for model ADO.
© ESO, 2012
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