Feeding Active Galaxies: Gas Dynamics from the Outskirts to the Very Center

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We analyze the gas dynamics of 16 nearby spiral galaxies. The H I gas
distributions and kinematics indicate that some properties of the atomic
gas correlate with the type of the AGN present. Furthermore, gas inflow
rates are derived as a function of radius and location within the disks
using combined H I and CO data.

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