Image Details

Choose export citation format:

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 D1.

Radial distributions of Σ*, ΣSFR, sSFR, and EWHα for various stellar-mass ranges. Gray lines represent individual galaxy profiles, with the radius sampled in steps of 0.2Re along the semimajor axis. Black lines indicate the location of the bulge for the same galaxy. Median profiles are color coded by stellar-mass range, blue (log(M*/M) ≤ 9.5), green (9.5 < log(M*/M) < 10), and red (log(M*/M) ≥ 10). Solid lines correspond to LSB galaxies, and dashed lines to HSB galaxies. Shaded areas reflect the errors of the median profile.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse