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THE ABUNDANCE PROPERTIES OF NEARBY LATE-TYPE GALAXIES. II. THE RELATION BETWEEN ABUNDANCE DISTRIBUTIONS AND SURFACE BRIGHTNESS PROFILES

  • Authors: L. S. Pilyugin, E. K. Grebel, I. A. Zinchenko, and A. Y. Kniazev

2014 The Astronomical Journal 148 134.

  • Provider: AAS Journals

Caption: Figure 1.

Resulting patterns of the bulge-disk decomposition of some of our target galaxies. Each galaxy is presented in two panels. Each upper panel ﹩x1﹩ shows the decomposition assuming a pure exponential for the disk (with “x” running from the letters a to i). The measured surface profile is plotted using circles. The bulge contribution is shown by a dotted line, the disk contribution by a dashed line, and the total (bulge + disk) fit by a solid line. Each lower panel ﹩x2﹩ shows the decomposition assuming a broken exponential for the disk. The bulge contribution is marked by a dotted line, the inner disk by a long-dashed line, the outer disk by a short-dashed line, and the total (bulge + disk) fit by a solid line.

(Supplemental data of this figure are available in the online journal.)

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