Image Details
Caption: Figure 9.
Top: the Gaia color–magnitude diagram for both the field sample and the 150 pc sample of young stars discussed in Gagné & Faherty (2018). We have zoomed in on the position of BD+60 1417 as an inset to show the closest isochrone. Bottom: Galaxy Evolution Explorer (GALEX) to Gaia (NUV−G) color vs. Gaia (G−GRP) for both the field sample and the 150 pc sample of 10–150 Myr young stars from Gagné & Faherty (2018). The position of BD+60 1417 is marked by a red five-point star.
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