The stellar corona-chromosphere connection - A comprehensive study of X-ray and Ca II IRT fluxes from eROSITA and Gaia

Open Access

Fig. 10

X-ray to bolometric flux ratio, $R_{I R T}^{'}$ $\[R_{\mathrm{IRT}}^{\prime}\]$ -index, and X-ray over IRT flux ratio as a function of the Rossby number for the sources detected in eRASS:5. The color coding is the same as in Fig. 4.

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