Mergers of Galaxies from an HI Perspective
| dc.creator | Hibbard, J. E. | |
| dc.date | 1999-10-25 | |
| dc.date | 1999-10-26 | |
| dc.date.accessioned | 2026-07-07T02:34:03Z | |
| dc.date.available | 2026-07-07T02:34:03Z | |
| dc.description | HI spectral line mapping studies are a unique probe of morphologically peculiar systems. Not only does HI imaging often reveal peculiarities that are totally unsuspected at optical wavelengths, but it opens a kinematic window into the outer dynamics of these systems that is unmatched at any other wavelength. In this review I attempt to summarize what we have learned from such studies, and what we may hope to learn from them in the future. | |
| dc.description | 10 pages, 5 figures, uses newpasp.sty, to appear in "Galaxy Dynamics: from the Early Universe to the Present", ASP Conf Series, eds F. Combes, G. Mamon and V. Charmandaris. Version with full-resolution figures available at http://www.cv.nrao.edu/~jhibbard/IAP15/iap15_review.ps.gz | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9910453 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9910453 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15093 | |
| dc.subject | Astrophysics | |
| dc.title | Mergers of Galaxies from an HI Perspective | |
| dc.type | text |