A tentative elementary model of quasars
| dc.creator | Moret-Bailly, Jacques | |
| dc.date | 2002-12-12 | |
| dc.date | 2002-12-24 | |
| dc.date.accessioned | 2026-07-25T18:52:34Z | |
| dc.description | A very simple model of quasar and Seyfert galaxy is obtained using the "Coherent Raman Effect on time-Incoherent Light" (CREIL) to explain a part of the observed redshifts. As its redshift is mostly provided by the CREIL, a QSO is not very far, its kernel may be a neutron star fed by the accretion of a disk, fed itself by the fall of many satellites. Disk and satellites are slowed by a relatively dense halo. The electric charges resulting of the friction of the disk produce flat lightnings, thus radio noise emitted mostly perpendicular to the disk, and X rays. The optical spectrum, including the shape of the spectral lines is explained without uncommon physics such as dark matter, by a splitting of the very wide lines resulting from simultaneous absorption and frequency shift, splitting due to a modulation of the redshift resulting from variations of a magnetic field. | |
| dc.description | 4 pages Version 2: Grammatical and typographical changes | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0212285 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0212285 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/59282 | |
| dc.subject | Astrophysics | |
| dc.title | A tentative elementary model of quasars | |
| dc.type | text |