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CHANG-ES XLI: Data Release 5—VLA C-configuration Images

  • Authors: René Walterbos, Theresa Wiegert, Michael Stein, Judith Irwin, Tanden Cook, Ancor Damas-Segovia, Jayanne English, Volker Heesen, Jiangtao Li, Scott Macdonald, Arpad Miskolczi, Michael Radica, Nathan Skeggs, Carlos Vargas, Q. Daniel Wang, Marek Weżgowiec, Jianghui Xu, Yang Yang

René Walterbos et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 6.

Plots of midplane cuts of the thermal fraction (left) and radio surface density (right) vs. SFR surface density. Data are from Table 7, except for the radio surface densities. Trend lines (dashed) are simple linear fits, and colored regions represent the 1σ confidence band on the regression, rather than the scatter in plot. Thermal fraction fits are (L band) fth,L  =   −0.44 ± 0.21) SFRSD + (0.156 ± 0.019) and (C band) fth,C  =   − (0.97 ± 0.46) SFRSD + (0.36 ± 0.04). Radio surface density fits are (L band) LSD(1020 W Hz−1 kpc−2)  =  (7.87 ± 0.85) SFRSD − (0.16 ± 0.08) and (C band) CSD(1020 W Hz−1 kpc−2)  =  (2.83 ± 0.32) SFRSD − (0.056 ± 0.029). Two AGN galaxies are labeled.

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