Search and analysis of giant radio galaxies with associated nuclei (SAGAN) - II. Molecular gas content of giant radio galaxies

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Fig. 9.

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Trends of specific star formation with other properties: the left plot shows the ratio of molecular gas to stellar mass as a function of sSFR. On the right we show the depletion time as a function of sSFR. Further details can be found in Sect. 5.1. The symbols in this plot are same as in Fig. 8.

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