Abstract
Quasar absorption spectra may offer a clue to the distribution of intergalactic matter clouds at cosmological distances. Essentially three types of absorption lines can be identified:
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1
- Broad absorption lines (or “throughs”) of highly ionized elements probably connected with the quasar phenomenon itselfes.
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2
- Heavy element systems, containing Ly (α if in the range of the spectrum, and stemming from gas oh near solar composition. They are characterized by a wide range of ionization states.
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3
- Numerous lines of the Ly (α “forest” on the short wavelength side of the Ly (α emission line and only a small contamination of metal or molecular lines.
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Müller, V., Mücket, J.P., Haubold, H.J., Gottlöber, S. (1989). Analysis of Absorption Lines in Quasar Spectra. In: Di Gesù, V., Scarsi, L., Crane, P., Friedman, J.H., Levialdi, S., Maccarone, M.C. (eds) Data Analysis in Astronomy III. Ettore Majorana International Science Series, vol 40. Springer, Boston, MA. https://doi.org/10.1007/978-1-4684-5646-2_20
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