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HAZMAT. III. The UV Evolution of Mid- to Late-M Stars with GALEX

  • Authors: Adam C. Schneider, and Evgenya L. Shkolnik

2018 The Astronomical Journal 155 122.

  • Provider: AAS Journals

Caption: Figure 6.

The median GALEX NUV to 2MASS J fractional flux density as a function of age for early-Ms (0.35–0.6 M; cyan) and mid- to late-Ms (0.08–0.35 M; red). Some symbols are slightly offset along the abscissa for differentiation purposes. Error bars represent inner quartiles as described in Section 4.1.

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