Galaxy Dynamics and the PNe Population
arXiv:astro-ph/0508642 · doi:10.1007/3-540-34270-2_42
Abstract
This review attempts to place the observations of extragalactic planetary nebulae in the context of galactic dynamics. From this point of view only the radial velocities of the PNe are important. We have built a specialised instrument to detect PNe in distant galaxies and measure their radial velocities in one step. This is explained in some detail, along with classical techniques for obtaining kinematic information. The review includes a vision of possible future developments in the field.
12 pages, 5 figures, ESO Workshop Planetary Nebulae beyond the Milky Way ESO, Garching, May 19-21, 2004 Planetary Nebulae beyond the Milky Way ESO, Garching, May 19-21, 2004
References in corpus (5)
- Planetary Nebulae as Standard Candles. XII. Connecting the Population I and Population II Distance Scales
- Dynamics of the Globular Cluster System Associated with M49 (NGC4472): Cluster Orbital Properties and the Distribution of Dark Matter
- The Planetary Nebula System and Dynamics in the Outer Halo of NGC 5128
- The Globular Cluster System of NGC 5128 II. Ages, Metallicities, Kinematics, and Formation
- The Planetary Nebulae Spectrograph: the green light for Galaxy Kinematics