The quasars are neutron stars embedded in clouds of hydrogen
| dc.creator | Moret-Bailly, Jacques | |
| dc.date | 2003-10-03 | |
| dc.date.accessioned | 2026-07-07T02:09:58Z | |
| dc.date.available | 2026-07-07T02:09:58Z | |
| dc.description | 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. | |
| dc.description | 7 pages | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0310087 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0310087 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6632 | |
| dc.subject | Astrophysics | |
| dc.title | The quasars are neutron stars embedded in clouds of hydrogen | |
| dc.type | text |