HAZMAT. III. The UV Evolution of Mid- to Late-M Stars with GALEX
Authors: Adam C. Schneider, and Evgenya L. Shkolnik
2018 The Astronomical Journal155122.
Provider: AAS Journals
Caption: Figure 7.
GALEX NUV to 2MASS J fractional flux density cumulative distribution functions for early-Ms (black) and mid- to late-type Ms (red) for all age groups. The shaded regions represent 1σ confidence intervals for each curve.