Fig. 4
Equivalent width of the broad Fe ii blend at 4570−4600 Å in our direct line of sight (black symbols) and at FOS4 (red symbols) with Gemini GMOS and VLT UVES in 2002−2015. This is an updated version of Fig. 6 in Mehner et al. (2012). The emission in our direct view of the star decreased by a factor of ~4, at FOS4 by only a factor of about ~2 between 2003 and 2015.
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