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The Structure and Kinematics of the Envelope Around U Ori from Iota Observations

  • Authors: Eugene A. Pluzhnik, Sam Ragland, Herve Le Coroller, William D. Cotton, William C. Danchi, Wesley A. Traub, and Lee Anne Willson

PLUZHNIK et al. 2009 The Astrophysical Journal 700 114.

  • Provider: AAS Journals

Caption: Figure 8.

Left: radial velocity distribution in the disk around U Ori (north top, east left). All available radial velocity measurements are marked with points in this figure. The best fit reflection-symmetric radial velocity pattern is shown, with grey for the average (−42 km s −1), white for receding (maximum with respect to average is +8 km s −1), and black for approaching (maximum with respect to average is −8 km s −1). The projections of the rotational axis, the polar outflow and some peculiar features Chapman et al. (1991) are also marked. Right: same as the left figure except for only data points used in the fitting procedure.

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