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Uncovering the origins of spiral structure through the measurement of pattern speeds and their radial variation

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Please use this identifier to cite or link to this item: http://hdl.handle.net/1928/9832

Uncovering the origins of spiral structure through the measurement of pattern speeds and their radial variation

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Title: Uncovering the origins of spiral structure through the measurement of pattern speeds and their radial variation
Author: Meidt, Sharon
Advisor(s): Rand, Richard
Committee Member(s): Rand, Richard
Henning, Patricia
Loomba, Dinesh
Roy, Mousumi
Department: University of New Mexico. Dept. of Physics & Astronomy
Subject: pattern speeds
spiral structure
LC Subject(s): Spiral galaxies--Structure.
Barred galaxies--Structure.
Density wave theory.
Resonance.
Degree Level: Doctoral
Abstract: At the intersection of galactic dynamics, evolution and global structure, unresolved issues in the nature and origin of spirals can be addressed through the characterization of the angular speeds of the patterns and their possible radial variation. In this thesis I describe the development, testing, and application of the Radial Tremaine-Weinberg (TWR) Method, a generalized version of the continuity-based TW method wherein the pattern speed is allowed to vary arbitrarily with radius. I will address the utility of, and caveats in applying, the TWR calculation together with a standard regularization technique in a series of tests on N-body simulations. The regularization, which smooths otherwise intrinsically noisy solutions based on a priori assumptions for the radial dependence of the pattern speed, proves to be essential for achieving the radial precision necessary for accurate measurement. I also present results from applications of the TWR method to observations of real galaxies, where the possible sources and sinks in the continuity equation are well understood. Using CO observations of the grand design galaxy M51, the TWR method reveals a heretofore un-measured inner spiral pattern speed for the bright two-armed spiral structure, with a value significantly higher than conventional estimates. In addition, the radial dependence implied in the TWR solution suggests a possible resonant link between the inner and outer regions of the bright spiral arms. These findings signify an advance in observational investigations into the nature and origin of grand-design spiral structure. By analyzing high-quality HI and CO data cubes available for four other spiral galaxies, the characteristic signatures of the processes that drive spiral structure are likewise identifiable; within this small sample, the first direct evidence for the presence of resonant coupling of multiple distinct patterns is found in some galaxies, while a simple single pattern speed is measured in others. I conclude with a summary of future avenues for investigation with the TWR method and propose additional modifications of the TW calculation with which the influence of bar and spiral structure on the evolution of galaxy disks can be directly characterized.
Graduation Date: July 2009
URI: http://hdl.handle.net/1928/9832


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