Star formation and gas flows in the centre of the NUGA galaxy NGC 1808 observed with SINFONI
arXiv:1611.07868 · doi:10.1051/0004-6361/201629440
Abstract
NGC 1808 is a nearby barred spiral galaxy which hosts young stellar clusters in a patchy circumnuclear ring with a radius of . In order to study the gaseous and stellar kinematics and the star formation properties of the clusters, we perform seeing-limited -band near-infrared integral-field spectroscopy with SINFONI of the inner . From the relation, we find a black hole mass of a few . We estimate the age of the young stellar clusters in the circumnuclear ring to be . No age gradient along the ring is visible. However, the starburst age is comparable to the travel time along the ring, indicating that the clusters almost completed a full orbit along the ring during their life time. In the central , we find a hot molecular gas mass of which, with standard conversion factors, corresponds to a large cold molecular gas reservoir of several , in accordance with CO measurements from the literature. The gaseous and stellar kinematics show several deviations from pure disc motion, including a circumnuclear disc and signs of a nuclear bar potential. In addition, we confirm streaming motions on scale that have recently been detected in CO(1-0) emission. Due to our enhanced angular resolution of , we find further streaming motion within the inner arcsecond, that have not been detected until now. Despite the flow of gas towards the centre, no signs for significant AGN activity are found. This raises the questions what determines whether the infalling gas will fuel an AGN or star formation.
arXiv comment19 pages, 19 figures, 3 tables; accepted for publication in Astronomy & Astrophysics
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