Image Details

Choose export citation format:

The FUSE Spectrum of PG 0804+761: A Study of Atomic and Molecular Gas in the Lower Galactic Halo and Beyond

  • Authors: Philipp Richter, Blair D. Savage, Bart P. Wakker, Kenneth R. Sembach, and Peter M. W. Kalberla

Richter et al. 2001 The Astrophysical Journal 549 281.

  • Provider: AAS Journals

Caption: Fig. 6.

Velocity profiles for the absorbing system at ﹩z_{\mathrm{abs}\,}=0.102﹩ associated with the background quasar PG 0804+761. The velocity scale is referenced to the redshift ﹩z=0.102﹩. The associated system is seen in H I, C III, and O VI and shows a two‐component structure in the strong lines of H I ﹩\lambda 1025.722﹩ and O VI ﹩\lambda 1031.926﹩ with the main component at ﹩0﹩ km s﹩^{-1}﹩ and a weaker component at ﹩\sim -45﹩ km s﹩^{-1}﹩. The profile for C III is not shown here because it is strongly blended by Galactic H2 R(0), 2–0 absorption.

Other Images in This Article
Copyright and Terms & Conditions