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Structural Components of NGC 5850
Published online by Cambridge University Press: 12 April 2016
Abstract
Here we present a study of the structural components of the barred galaxy NGC 5850 using U, B and I photometry. After subtracting a bulge+disk model from the observed image, we obtain the bar and other non-axisymmetric structures. We determine the position of the ILR from the ellipticity and position angle profiles of the isophotes.
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- Copyright © Astronomical Society of the Pacific 1996