2003/10/03 by Jacques Moret‐Bailly, Jacques Moret-Bailly, Moret-Bailly, Jacques
Physics and Astronomy · #Astro and Planetary Science #Astrophysical Phenomena and Observations #Astrophysics and Star Formation Studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0310087
7 pages
arxiv created 2003/10/03 · arxiv updated 2009/12/01
The accretion of a cloud of hydrogen at the surface of a small, heavy star produces a high energy mostly dissipated by electromagnetic radiation. The combination of the absorption and the redshift of this radiation by hydrogen explains all spectral observations: shapes of the broad lines, and their anti-correlation with the radio-loudness, lack of lines in front of the Lyman forest, value zb = 0.062 of the periodicity of the redshifts, correlation of a high redshift with a thermal spectrum attributed to dust. These properties are deduced from usual laws of physics without new parameters, they do not require any non baryonic matter.