Image Details
Caption: Figure 2.
The results of isophote analysis for ESO 119-055 in the r-band (two left plots) and the surface brightness profile azimuthally averaged with the outer disk’ line-of-nodes orientation and inclination. Two fitted exponential laws for the inner and outer stellar disks are overposed, their parameters are: μr = 21.2 + 1.086R″/19″ for the inner one and μr = 22.2 + 1.086R″/30″ for the outer one.
© 2026. The Author(s). Published by the American Astronomical Society.