2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/3223Results from kinematic observations of the central regions of spiral galaxies are reviewed, with particular emphasis on starburst and AGN hosts. While morphological studies lead to important insight, a more complete understanding of the physical processes that drive the evolution of the central regions can be achieved with measurements of the kinematics of gas and stars. Here, a variety of observational techniques at different wavelengths is critically discussed, and specific areas of interest are highlighted, such as inflow in barred galaxies and the origin of nuclear spiral arms. A brief discussion of a number of case studies is presented to illustrate recent progress.Invited review, to appear in The Central kpc of Starbursts and AGN: the La Palma Connection, eds. J. H. Knapen, J. E. Beckman, I. Shlosman, and T. J. Mahoney (ASP: San Francisco), Vol. 249. 18 pages latex, includes 9 postscript figures. Uses newpasp.sty (included)AstrophysicsKinematics in the Central Kiloparsec of Spiral Galaxiestext