Abstract
I briefly 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 σ-drops and counter-rotating nuclear disks as probed via integral-field spectroscopy.
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Emsellem, E. (2004). Bar-Driven Fueling of Galactic Nuclei: A 2D View. In: Block, D.L., Puerari, I., Freeman, K.C., Groess, R., Block, E.K. (eds) Penetrating Bars through Masks of Cosmic Dust. Astrophysics and Space Science Library, vol 319. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-2862-5_11
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DOI: https://doi.org/10.1007/978-1-4020-2862-5_11
Publisher Name: Springer, Dordrecht
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