Abstract
Among the many spectral lines falling in the ultraviolet are the resonance doublets of the highly ionized species O VI, N V, C IV, and Si IV. By using both space-based UV observations and ground-based optical observations, these lines can be used to trace diffuse astrophysical plasma over a large fraction of the age of the Universe. In this paper we discuss observations of these absorption lines in damped Lyman-α systems at z≈2–3, using the UVES spectrograph on the VLT in Chile.
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P. Petitjean is also at LERMA, Observatoire de Paris.
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Fox, A.J., Petitjean, P., Ledoux, C. et al. Studying hot gas using the ultraviolet: High ions in galactic halos. Astrophys Space Sci 320, 27–30 (2009). https://doi.org/10.1007/s10509-007-9722-2
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DOI: https://doi.org/10.1007/s10509-007-9722-2