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The Stellar Disk Thickness of Low Surface Brightness Galaxies

  • Authors: D. Bizyaev and S. Kajsin

Bizyaev & Kajsin 2004 The Astrophysical Journal 613 886.

  • Provider: AAS Journals

Caption: Fig. 9.

Same as Fig. 1, but for UGC 9556. The isophotes correspond to 20.5, 21, 21.5, 22, 22.5, 23, 23.5, 24, 24.5, 25, 26, and 26.7 mag arcsec−2. The diagonal feature in the bottom panel is a remainder of a bright satellite track.

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