2003/07/08 by Jacques Moret‐Bailly, Jacques Moret-Bailly, Moret-Bailly, Jacques
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #Electrical and Electromagnetic Research #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0307140
3 pages
arxiv created 2003/07/08 · openalex publication_date 2003/07/08 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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.