New views on bar pattern speeds from the NUGA survey

(10) MPE Garching); (2) Obs. de Madrid; (3) Obs. de Paris/LERMA; (4) Harvard-Smithsonian CfA Cambridge; (5) MPIA Heidelberg; (6) Rutgers NJ; (7) Un. Koln; (8) IRAM Granada; (9) IRAM Grenoble; A. Eckart (7)

arxiv: 0811.1971 · v1 · submitted 2008-11-12 · 🌌 astro-ph

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)

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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 (4) Harvard-Smithsonian CfA Cambridge (5) MPIA Heidelberg (6) Rutgers NJ (7) Un. Koln (8) IRAM Granada (9) IRAM Grenoble (10) MPE Garching)

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keywords nugagalaxiespatternspeedschallengingcircumnuclearcontextcurrent

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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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New views on bar pattern speeds from the NUGA survey

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