Fig. 9.
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Location of the AT 2018bwo progenitor in the HR diagram. MESA single stellar evolution tracks are shown for stars between 9 and 13 M⊙. The main sequence is marked with a thicker line. Different markers represent progenitor parameters using different models (see Table 4). The insert shows a zoomed in region around the progenitor location, along with a finer grid of models.
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