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Bar-Driven Fueling of Galactic Nuclei: A 2D View
[chapter]
2004
Astrophysics and Space Science Library
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I discuss evidences for bar-driven gas fueling in the central regions of galaxies, focusing on scales down to about 10 pc. I thus mention the building of inner disks, and the link with resonances, as well as the corresponding kinematic signatures such as sigma-drops and counter-rotating nuclear disks as probed via integral-field spectroscopy.
doi:10.1007/978-1-4020-2862-5_11
fatcat:plxt2ajkw5avtifhvfznrzxdwu