Fig. 7.
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Nebular oxygen abundance versus stellar mass for the six spectroscopically confirmed TDGs. No oxygen abundance is available for Arp72c. The fundamental relation for star-forming SDSS galaxies with log M* > 8.5 from Duarte Puertas et al. (2022) is shown as a black solid line. The gray shaded range marks the rms spread in the best-fit relation. Dwarf galaxy relation from Berg et al. (2012) is shown in pink.
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