Fig. 3
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Temporal profile of stellar accretion rates for the nine discs studied in this work (Table 1) when λ = 3. Additionally, cases with λ = 1.6, λ = 17, and purely viscously evolving scenarios for disc 5 are also shown. Various symbols correspond to observed values: black cross markers: Batalha & Basri (1993); Galli et al. (2015); Nuernberger et al. (1997); Andrews et al. (2018); Alcalá et al. (2014); Green cross markers: Andrews et al. (2018); Erickson et al. (2011); Andrews et al. (2010); Blue cross markers: Herczeg & Hillenbrand (2014); Garufi et al. (2020); Sicilia-Aguilar+2020: Sicilia-Aguilar et al. (2010).
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