Figure 2 from THE ABUNDANCE PROPERTIES OF NEARBY LATE-TYPE GALAXIES. II. THE RELATION BETWEEN ABUNDANCE DISTRIBUTIONS AND SURFACE BRIGHTNESS PROFILES

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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 2.

Quality of the surface brightness profile fit obtained via the bulge-disk decomposition. The mean deviation ﹩{{\sigma }_{{\rm BED}}}﹩ of the fit assuming a broken exponential disk is plotted vs. the mean deviation ﹩{{\sigma }_{{\rm PED}}}﹩ of the fit assuming a pure exponential disk. The dotted line shows equal values.

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