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SDSS-IV MaNGA: Distinct Structural Growth and Star Formation in Low and High Surface Brightness Disks

  • Authors: Mengting Shen, Jun Yin, Hassen M. Yesuf, Lei Hao, Jiafeng Lu, Lin Lin, Chong Ge, Junfeng Wang, Shiyin Shen, Yu Rong

Mengting Shen et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 7.

The radial profile of Σ* as a function of R/Re and the cumulative M* as a function of physical radius R in different stellar-mass ranges. Blue, green, and red correspond to the mass ranges ≤109.5, 109.5–1010, and ≥1010 M, respectively. Within each mass range, the solid line represents the median profile of LSB galaxies, the dashed line for HSB galaxies, and the dotted line for large-size galaxies. Shaded areas denote the errors associated with each median profile. The number of LSB and HSB galaxies in each stellar-mass range is listed in the legend.

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