Abstract
In the Friedmann regression analysis the absorption lines of the Lyman α forest of quasars are identified with the crossings of the quasar light with hydrogen filaments located in the walls of a universal bubble structure. An analysis of 21 quasar spectra with 1360 absorption lines restricts the cosmological parameters of homogenous isotropic world models to those of a Friedmann Lemaitre model with best fit values of Ω0 = 0,014 ± 0.002 and λ0 = Λc 2/3H 0 2 = 1.080 ± 0.006.
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© 1994 Springer Science+Business Media Dordrecht
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Hoell, J., Priester, W. (1994). The Lyman α Forest and the Universal Bubble Structure. In: Wamsteker, W., Longair, M.S., Kondo, Y. (eds) Frontiers of Space And Ground-Based Astronomy. Astrophysics and Space Science Library, vol 187. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0794-5_99
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DOI: https://doi.org/10.1007/978-94-011-0794-5_99
Publisher Name: Springer, Dordrecht
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