Fourier Analysis of Isolated Galaxies in the Context of the AMIGA Project

Details Fourier Analysis of Isolated Galaxies in the Context of the AMIGA Project Fourier Analysis of Isolated Galaxies in the Context of the AMIGA Project

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21344310d&link_type=abstract

American Astronomical Society, AAS Meeting #213, #443.10; Bulletin of the American Astronomical Society, Vol. 41, p.325

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We present the results of Fourier analysis of a representative sample (N 100) of isolated galaxies in the local Universe. The photometric study focuses on Sb-Sc morphological types because they are the most common among our population of isolated galaxies. We are using SDSS i-band images and measure the spiral strength and bar strength (about 60% of our sample are barred). The results of our analysis are also evaluated in relation to a large set of parameters obtained from a bulge-disk-bar decomposition for the same sample of isolated disk galaxies. Our work is an integral part of the international AMIGA (Analysis of the interstellar Medium of Isolated GAlaxies) project.

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