New views on bar pattern speeds from the NUGA survey
V. Casasola (1), S. Garcia-Burillo (2), F. Combes (3), L. K. Hunt (1),, M. Krips (4), E. Schinnerer (5), A. J. Baker (6), F. Boone (3), A. Eckart, (7), S. Leon (8), R. Neri (9), L. J. Tacconi (10). ((1) INAF-IRA Firenze, (2), Obs. de Madrid, (3) Obs. de Paris/LERMA

TL;DR
This paper reviews initial findings on bar pattern speeds from the NUGA survey, highlighting the diversity of molecular circumnuclear structures and their implications for galaxy dynamical models.
Contribution
It provides new insights into bar pattern speeds and emphasizes the need to refine galaxy dynamical models based on diverse molecular morphologies.
Findings
Diverse molecular circumnuclear morphologies observed
Implication that current dynamical models need refinement
Preliminary results suggest complex bar pattern speed behaviors
Abstract
We present a review on bar pattern speeds from preliminary results in the context of the Nuclei of Galaxies (NUGA) project. The large variety of molecular circumnuclear morphologies found in NUGA is a challenging result that implies the refinement of current dynamical models of galaxies.
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Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Scientific Research and Discoveries
