Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-26T03:40:52.875Z Has data issue: false hasContentIssue false

On the Interpretation of QSO Absorption Lines

Published online by Cambridge University Press:  03 August 2017

V. Müller
Affiliation:
Zentralinstitut für Astrophysik der AdW der DDR, Potsdam, DDR - 1591
J. P. Mücket
Affiliation:
Zentralinstitut für Astrophysik der AdW der DDR, Potsdam, DDR - 1591
S. Gottlöber
Affiliation:
Zentralinstitut für Astrophysik der AdW der DDR, Potsdam, DDR - 1591
H. J. Haubold
Affiliation:
Zentralinstitut für Astrophysik der AdW der DDR, Potsdam, DDR - 1591

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

OSO absorption spectra may offer a clue to the distribution of intervening matter clouds at z = 0 … 3. We tackle 1) the question of the occurrence of metal absorption lines of different ionisation levels in the same redshift systems by investigating the radiation transport through an inhomogeneous temperature profile; 2) the clustering properties of the lines of the Lyα forest by a correlation analysis of 9 published high-resolution QSO-spectra with the result of a certain contribution of metal absorption lines as well as marginally significant positive correlation regions ξ ≈ 0.3.

Type
Appendix 1: Poster Papers
Copyright
Copyright © Reidel 1988 

References

Doroshkevich, A.G., Mücket, J.P.: 1985, Sov. Astron. Lett. 11, 137.Google Scholar
Müller, V., Mücket, J.P., Haubold, H.J.: 1987 Astron. Nachr. 308, 177.CrossRefGoogle Scholar
Mücket, J.P., Müller, V.: 1987 PRE-ZIAP 87-09, (subm. for publication).Google Scholar