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Adaptive Optics Echelle Spectroscopy of [Fe II] 1.644 μm in the RW Aur Jet: A Narrow Slice Down the Axis of the Flow

  • Authors: Patrick Hartigan and Lynne Hillenbrand

HARTIGAN & HILLENBRAND 2009 The Astrophysical Journal 705 1388.

  • Provider: AAS Journals

Caption: Figure 3.

Same as Figure 2 but for the FWHM of the [Fe ii] 1.644 μm line profiles. The emission line widths are resolved for all points in the figure, and decrease monotonically with distance from the star.

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