Certainly, we cannot ignore the possibility that transit events may be responsible for the variations observed in some of these loBALs. For example, the presence of a P V BAL indicates that the C IV BAL is highly saturated, as evidenced by the C IV/P V optical depth ratio being greater than ∼100. This finding is supported by studies conducted by Hamann (1998), Leighly et al. (2009), Leighly, Dietrich & Barber (2011), and Borguet et al. (2012). Expanding on these findings, Capellupo et al. (2014) argue that the variability observed in the P V and saturated C IV BALs strongly supports the transit scenario.

Transit Events as a Potential Cause for Variability in loBALs

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