Image Details
Caption: Fig. 1.
Snapshot of density and poloidal velocity vectors illustrating the jet and disk wind for all cases of disk density variation. Gray scale (logarithm of the number density measured in cm−3; ≤8.26 is white and ≥10.46 is black) and velocity scale are consistent for all frames. The panels, from top to bottom, are the low‐density case (at ﹩t=147﹩ days), the baseline case (at ﹩t=136﹩ days), and the high‐density case (at ﹩t=137﹩ days). In each panel, the equatorial plane is along the bottom, and the star is at bottom center.
© 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.