2003/10/16 by Jacques Moret‐Bailly, Jacques Moret-Bailly, Moret-Bailly, Jacques
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics (astro-ph) #FOS: Physical sciences #Pulsars and Gravitational Waves Research #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0310452
V2: complete e reference and correct a visible mistake (3 words)
openalex publication_date 2003/10/16 · arxiv created 2003/11/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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. As a large part of the redshift is intrinsic, the quasars are not extremely far, the may be the missing "accretor isolated neutron stars". These properties are deduced from usual laws of physics without new parameters, they do not require any non baryonic matter.