Bar-driven fueling of galactic nuclei: a 2D view

Eric Emsellem

doi:10.1007/978-1-4020-2862-5_11

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arXiv · astro-ph/0409625

Bar-driven fueling of galactic nuclei: a 2D view

Eric Emsellem

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Abstract

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.

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Eric Emsellem. 2004-09-27. Bar-driven fueling of galactic nuclei: a 2D view. https://doi.org/10.1007/978-1-4020-2862-5_11

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