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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 4.

Radial offsets in the sSFR and gas-phase metallicity for LTGs in close S + S and S + E pairs, relative to their matched isolated controls. The top-left and top-right panels show ﹩{\rm{\Delta }}\mathrm{log}({\rm{sSFR}})﹩ and ﹩{\rm{\Delta }}\mathrm{log}({\rm{O}}/{\rm{H}})﹩ when the pairs are divided into subsamples by companion galaxy mass, respectively. The bottom-left and bottom-right panels present the corresponding ﹩{\rm{\Delta }}\mathrm{log}({\rm{sSFR}})﹩ and ﹩{\rm{\Delta }}\mathrm{log}({\rm{O}}/{\rm{H}})﹩ when the pairs are divided by the stellar mass of the target galaxy.

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