Symmetry for Nearest Stars and N-body Problem with Delay for Interaction
| dc.creator | Faizullin, Rashid | |
| dc.date | 1995-08-11 | |
| dc.date.accessioned | 2026-07-07T02:19:59Z | |
| dc.date.available | 2026-07-07T02:19:59Z | |
| dc.description | In the present paper some geometrical and mechanical regularities are introduced, which constitute certain puzzles of distribution of the nearest stars of $O,B,AO$ classes (brighter than $6.0^m$) and of the brightest galactic objects; the regularities appear when considering in the natural, moment related ($l,b$), ($α,δ$), ($λ,β$) coordinate planes. Also, there are some efforts for deduction these cases from Newton law with delay for gravitational interaction. | |
| dc.description | LaTeX, 5 figures in LaTex, in the Proceedings of Int.Conf. "Groups in analisys and geometry" Omsk 1995 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9508053 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9508053 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10082 | |
| dc.subject | Astrophysics | |
| dc.title | Symmetry for Nearest Stars and N-body Problem with Delay for Interaction | |
| dc.type | text |