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Radial Distributions of Star Formation and Gas-phase Metallicity in Spiral–Elliptical Galaxy Pairs

  • Authors: Cailu Shi, 彩璐 石, Shuai Feng, 帅 冯, Shiyin Shen, 世银 沈, Linlin Li, 林林 李, Wenyuan Cui, 文元 崔, Guozhen Hu, 国真 胡

Cailu Shi et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 3.

Radial profiles of ﹩\mathrm{log}\,\rm{sSFR}\,﹩ (top) and ﹩12+\mathrm{log}(\rm{O}\,/\,\rm{H})﹩ (bottom) for spiral galaxies in close S + S (blue) and S + E (red) pairs. Left panels: median radial profiles of paired galaxies (solid lines) and their matched isolated controls (dashed lines), plotted as a function of normalized radius (R/Re). Right panels: radial offsets between paired galaxies and their matched isolated controls.

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