The distribution of interstellar C IV in the galaxy

Astronomy and Astrophysics – Astronomy

Scientific paper

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Cosmic Plasma, Galactic Structure, Iue, Milky Way Galaxy, Ultraviolet Astronomy, Absorption Spectra, B Stars, Carbon, Disks (Shapes), Ion Density (Concentration), Nitrogen, Oao 3, Oxygen, Silicon, Stellar Spectra

Scientific paper

Some high dispersion spectra of 13 halo and disc stars were reduced and column densities of C IV presented. The galactic distribution of C IV is discussed and, combining the data with other published measurements, a mean exponential scale height of 3 + 2 -1 kpc and disk space density no = 8.5 x 10 to the minus 9th power cu cm are derived. The results were compared with Copernicus O VI data. Strengths and profiles of Si IV, C IV and N V from International Ultraviolet Explorer data were also compared for a few representative lines of sight. N V/O VI ratios imply log T 5.5, while SI IV/C IV (including the value for the whole halo towards 3C 273) require 4.80 less than Log T less than 4.95.

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