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Galaxy Dynamics and the PNe Population

Authors: Douglas, Nigel G.;

Galaxy Dynamics and the PNe Population

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

Country
Netherlands
Related Organizations
Keywords

NGC-5128, RADIAL-VELOCITIES, GLOBULAR-CLUSTER SYSTEM, HALO, Astrophysics (astro-ph), DARK-MATTER, FOS: Physical sciences, KINEMATICS, PLANETARY-NEBULA SYSTEM, MASS, Astrophysics

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    popularity
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    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green