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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 11.

The median GALEX FUV/NUV fractional flux density for young M stars (TW Hya, β Pic, and Tuc-Hor) and field-age M stars as a function of mass. Some symbols are slightly offset along the abscissa for differentiation purposes. Error bars represent inner quartiles.

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