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2001MNRAS.328.1064N - Mon. Not. R. Astron. Soc., 328, 1064-1080 (2001/December-3)
The kinematics of lopsided galaxies.
NOORDERMEER E., SPARKE L.S. and LEVINE S.E.
Abstract (from CDS):
The lopsidedness in our models is most pronounced in the models where the halo provides a relatively large fraction of the total mass at small radii. This may explain why the gas shows lopsidedness more frequently in late-type galaxies, which are dominated by dark matter. Surfaces of section show large regions of irregular orbits in the models where the halo density is low. This may indicate that these models are unstable.
Abstract Copyright: The Royal Astronomical Society
Journal keyword(s): galaxies: formation - galaxies: individual: NGC 4395 - galaxies: kinematics and dynamics - galaxies: structure - dark matter
Simbad objects: 3
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