NGC 488: Has its massive bulge been build up by minor mergers?
| dc.creator | Fuchs, Burkhard | |
| dc.date | 1997-08-04 | |
| dc.date.accessioned | 2026-07-07T02:23:57Z | |
| dc.date.available | 2026-07-07T02:23:57Z | |
| dc.description | Using recent observations of the kinematics of the disk stars the dynamical state of the disk of NGC 488 is discussed. The disk is shown to be dynamically `cool', so that NGC 488 cannot have experienced many -- even minor -- mergers in the past. | |
| dc.description | Latex, 6 pages, 5 figures, to appear in A&A | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9708029 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9708029 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11446 | |
| dc.subject | Astrophysics | |
| dc.title | NGC 488: Has its massive bulge been build up by minor mergers? | |
| dc.type | text |