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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents

ID: 709879.0, MPI für Astronomie / Publikationen_mpia
Interlocking resonance patterns in galaxy disks
Authors:Font, J.; Beckman, J. E.; Querejeta, M.; Epinat, B.; James, P. A.; Blasco-herrera, J.; Erroz-Ferrer, S.; Pérez, I.
Date of Publication (YYYY-MM-DD):2014
Title of Journal:The Astrophysical Journal Supplement Series
Issue / Number:1
Start Page:id. 2 (30 pp)
Audience:Not Specified
Abstract / Description:We have developed a method for finding dynamical resonances in disk galaxies using the change in sense of the radial component of the in-plane velocity at a resonance radius. Using simulations we show that we would expect to find these changes at corotation radii with a weaker effect at the Lindblad resonances. The method works well with observations at high spectral and angular resolutions, and is suited to the analysis of two-dimensional velocity fields in Halpha from Fabry-Perot spectroscopy. We find clear indications of resonance effects in the disk velocity fields of virtually all of the 104 galaxies. The number of resonance radii detected ranges from one to seven, with a median of four. The frequency curves Omega, Omega ± kappa/2, Omega ± kappa/4 against radius for all the galaxies led us to discover a pattern in over 70% of the sample: given two pattern speeds, say Omega1 and Omega2, the OLR of Omega1 coincides with the corotation of Omega2, and the inner 4:1 resonance of Omega2 coincides with the corotation of Omega1. Although the second coincidence has been predicted, a prediction of this double coincidence is not found in the literature. This pattern is found once in 42 of the galaxies, twice in a further 26, three times in 5, and even four times in 1 galaxy. We also compute the ratio of corotation radius to bar length where we have sufficient image quality, finding a mean value of 1.3, and a shallow increase toward later type galaxies.
Free Keywords:galaxies: fundamental parameters; galaxies: kinematics and dynamics; galaxies: spiral; galaxies: structure; techniques: interferometric
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0067-0049 %R 10.1088/0067-0049/210/1/2
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