Theory of the quantification of the redshifts
| dc.creator | Moret-Bailly, Jacques | |
| dc.date | 2003-07-08 | |
| dc.date.accessioned | 2026-07-07T02:08:56Z | |
| dc.date.available | 2026-07-07T02:08:56Z | |
| dc.description | 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. | |
| dc.description | 3 pages | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0307140 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0307140 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6254 | |
| dc.subject | Astrophysics | |
| dc.title | Theory of the quantification of the redshifts | |
| dc.type | text |