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The Evolution of Flare Activity with Stellar Age

  • Authors: James R. A. Davenport, Kevin R. Covey, Riley W. Clarke, Austin C. Boeck, Jonathan Cornet, and Suzanne L. Hawley

2019 The Astrophysical Journal 871 241.

  • Provider: AAS Journals

Caption: Figure 5.

Specific flare rate (R35), evaluated at an energy of log E = 35 erg as a function of the stellar mass and Rossby number (top), and the observed stellar rotation and color (bottom). The sample is the same as in Figure 4.

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