Figure 4 from HAZMAT. III. The UV Evolution of Mid- to Late-M Stars with GALEX

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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 4.

Stacked histograms of the GALEX FUV to 2MASS J flux density ratio for early (left) and mid- to late- (right) objects in this sample. The red histograms represent detections, while upper limits are shown in blue. Dashed lines represent the median values given in Table 4.

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