Central Rotation Curves of Galaxies
| dc.creator | SOFUE, Yoshiaki | |
| dc.date | 2000-10-30 | |
| dc.date.accessioned | 2026-07-07T01:56:16Z | |
| dc.date.available | 2026-07-07T01:56:16Z | |
| dc.description | We emphasize the use of high-resolution CO line observations to derive central rotation curves of galaxies. We present an example for high-resolution interferometer observations of NGC 3079, and discuss the PV diagram and derived rotation curve. The CO central rotation curves are combined with the outer curves from \ha and HI-line observations to obtain total RC. We show that well resolved RCs for massive galaxies generally start from non-zero velocities at the nucleus. | |
| dc.description | 4 pages, 4 figures, in "Galaxy Disks and Disk Galaxies", ASP Conf. Series, Vatical Conf. Rome 2000, eds. J. Funes, and E.M. Corsini | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0010595 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0010595 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1936 | |
| dc.subject | Astrophysics | |
| dc.title | Central Rotation Curves of Galaxies | |
| dc.type | text |