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Far Ultraviolet Spectroscopic Explorer Observations of RX J0513.9−6951

  • Authors: J. B. Hutchings, A. P. Cowley, R. Mann, P. C. Schmidtke, and D. Crampton

Hutchings et al. 2005 The Astronomical Journal 129 2792.

  • Provider: AAS Journals

Caption: Fig. 6.

Profiles of the Lyman absorption lines least contaminated by airglow emission and H2 absorption. Fluxes are in ergs cm−2 s−1 Å−1. Each line is identified by its rest wavelength and shifted vertically by ﹩2\times 10^{-14}﹩ to provide separation from the mean profile (thick solid line). Note the flat‐bottomed saturated absorption profiles and the large width in velocity.

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