Titlebook: Barred Galaxies and Circumnuclear Activity; Proceedings of the N Aage Sandqvist,Per Olof Lindblad Conference proceedings 1996 Springer-Verl

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https://doi.org/10.1007/978-3-031-17933-4al region is associated with a dense molecular gas disk, in which the majority of gas is concentrated in a rotating molecular ring. Outflow structures like the radio lobe is associated with rotating molecular gas at high speed, consistent with a twisted magnetic cylinder driven by accretion of a rotating gas disk.

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The barred galaxy NGC 1530, identify with large scale shocks observed in hydrodynamic simulations. Although hydrodynamical models are generally used to constrain the mass model, the observations could in turn be used to find a better ISM descriptor.

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A circumnuclear molecular torus in NGC 1365, 5″ is the dominant feature. Molecular emission is also seen coming from various dust streamers in the bar of the galaxy. The velocity field of the molecular region agrees well with predictions of models of gas streaming in the bar and nuclear region.

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Radio continuum and molecular gas in the Galactic Center,al region is associated with a dense molecular gas disk, in which the majority of gas is concentrated in a rotating molecular ring. Outflow structures like the radio lobe is associated with rotating molecular gas at high speed, consistent with a twisted magnetic cylinder driven by accretion of a rotating gas disk.

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Conference proceedings 1996etical papers describe their evolution, the dynamics as well as fundamental physical effects near their nuclei. Other contributions cover numerical and observational aspects and thus represent a very active area in astrophysics. The centre of our galaxy was also amply dealt with. The collection addresses researchers as well as graduate students.

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