Fig. 16
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Accretion rates from spectral line luminosities in M⊙ yr−1 for B243, B268, and B275. Each bracketed column is for a given line and shows the rates for all epochs separately. The values should be considered with care given the uncertainties associated with the applied method (see text), but they are typically ~10−6 M⊙ yr−1 for B243 and B268, and up to ~10−5 M⊙ yr−1 for B275.
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