Internal Kinematics of Microstructures and Implications
| dc.creator | Miranda, Luis F. | |
| dc.date | 2003-10-14 | |
| dc.date.accessioned | 2026-07-07T02:10:23Z | |
| dc.date.available | 2026-07-07T02:10:23Z | |
| dc.description | High resolution images at different wavelengths show the common presence of structures and microstructures in planetary nebulae (PNe), which are not well incorporated to the existing models for the formation of these objects. We summarize how studies of the internal kinematics, combined with the information provided by high resolution images, may help to establish the nature and possible origin of the observed structures as well as to provide information about the physical processes involved in the formation and evolution of PNe. | |
| dc.description | 7 pages, 4 figures; to appear in "Asymmetrical Planetary Nebulae III" editors M. Meixner, J. Kastner, N. Soker, & B. Balick (ASP Conf. Series) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0310369 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0310369 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6722 | |
| dc.subject | Astrophysics | |
| dc.title | Internal Kinematics of Microstructures and Implications | |
| dc.type | text |