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Direct Spectroscopic Observations of Clumping in O-Star Winds

  • Authors: Sébastien Lépine and Anthony F. J. Moffat

LÉPINE & MOFFAT 2008 The Astronomical Journal 136 548.

  • Provider: AAS Journals

Caption: Figure 5.

Comparison between the normalized mean profiles of the emission lines and the observed dispersion in the line profile, as a function of wavelength. Mean (thick) lines and dispersion (thin) lines are superposed on each plot, with the amplitude of the dispersion multiplied by a factor of 35 (hence a dispersion level of 0.35 on the plot actually corresponds to a dispersion amplitude of 0.01 in normalized flux units).

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