A closer look at the young stellar group around Sh 2-295

Open Access

Fig. 5

W(Li) from the 6708 Å line vs T_eff and spectral type. Symbols and colours are the same as in Fig. 4. Grey lines are polynomial fits for observed data in other young clusters: Sco-Cen (10–16 Myr), IC2602 (45 Myr), and Pleiades (125 Myr) – see Pecaut & Mamajek (2016) and references therein. The orange line represents the expected curve for a population of ${8.1}_{- 3.8}^{+ 2.1}$ $Mathematical equation: $\[8.1_{-3.8}^{+2.1}\]$$ Myr, as calculated by EAGLES v2.

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