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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S245(3)

DOI: 10.1017/s1743921308017808

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Feeding black holes: tracing gas flows from the outskirts to the centers of galaxies

Journal article published in 2007 by S. Haan, E. Schinnerer ORCID, C. G. Mundell, F. Combes ORCID, S. García-Burillo, E. Emsellem
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe analyzed the distribution and kinematics of the atomic gas (HI) in 16 nearby spiral galaxies. Our results indicate that the morphology of the atomic gas and dynamically disturbed outer disks correlate with the AGN type present (Seyfert, LINER). From the combined HI and CO data (from the NUGA project), 2-dimensional maps of the gas flow are computed and gas inflow rates are derived as a function of radius within the disks.

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