Theory of the quantification of the redshifts

The quantification of the redshifts of the lines observed in the spectra of the quasars and the galaxies (the redshifts of their lines have some of the values given by the formula z=a+0.062m where a depends on the object, and m is an integer), the density of the lines, result from a purely spectrosc...

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Bibliographic Details
Published inarXiv.org
Main Author Moret-Bailly, Jacques
Format Paper
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 08.07.2003
Subjects
Galaxies
Line spectra
Quasars
Spectrum analysis
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Summary:The quantification of the redshifts of the lines observed in the spectra of the quasars and the galaxies (the redshifts of their lines have some of the values given by the formula z=a+0.062m where a depends on the object, and m is an integer), the density of the lines, result from a purely spectroscopic effect. The explanation requires only standard spectroscopy, a nearly homogeneous halo of atomic hydrogen, and a magnetic field.
ISSN:2331-8422