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Gas flow and dark matter in the inner parts of early-type barred galaxies I. SPH simulations and comparison with the observed kinematics

Perez, I; Fux, Roger; Freeman, Kenneth


The dynamical simulations run in the potential derived from the light distribution of 5 late-type barred spiral galaxies were discussed. Simulations were run for potentials obtained from the I-band light distribution and from the composite of a H-band images at the centre and I-band image in the outer isophotes. Such models show differences in the gas distribution resulting from the higher dust absorption in the central regions of the I-band image. It was found that the gravitational field in...[Show more]

CollectionsANU Research Publications
Date published: 2004
Type: Journal article
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361:20040333


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