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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 8.

GALEX FUV to 2MASS J fractional flux density as a function of age for all objects in this sample. Detections are shown as filled red circles, while upper limits are blue triangles. Some symbols are slightly offset along the abscissa for differentiation purposes. The large cyan diamonds represent the median flux density ratios for each age group. Error bars on the medians represent inner quartiles as described in Section 4.1.

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