Quantifying secular evolution through structural decomposition
Published in Proceedings of the International Astronomical Union • Aug 1, 2012
NobleIDNI5P26W97R57S01
Authors:
L. S. Kelvin
Abstract
Abstract Structure within a galaxy is not random, instead emerging as a direct function of its evolutionary path. It is thought that secular evolutionary processes leave behind distinct structural tracers in the form of bars, pseudo-bulges and rings. We have developed a robust automated structural a...
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