Figure 3 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 3.

Comparison between disk scale lengths in the ﹩W1﹩ ﹩WISE﹩ band with the isophotal wavelength at 3.4 μm (this study) and in the 3.6 μm band of the Spitzer Survey of Stellar Structure in Galaxies (Muñoz-Mateos et al. 2013) (see the text). The dotted line shows equal values.

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