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Stellar Activity in the Broadband Ultraviolet

  • Authors: K. Findeisen, L. Hillenbrand, and D. Soderblom

Findeisen, Hillenbrand, & Soderblom 2011 The Astronomical Journal 142 23.

  • Provider: AAS Journals

Caption: Figure 4.

RHK vs. UV − V diagrams of our volume-limited Hipparcos sample. The left panel only shows stars with V + 12.03( BV) < 15.5, where our FUV observations were complete. In the left panel, red points have BV > 0.7, green points have 0.6 < BV < 0.7, and blue points have BV < 0.6. In the right panel, red points have BV > 0.9, green points have 0.8 < BV < 0.9, and blue points have BV < 0.8. The ellipses at the top right of either panel show the median errors along each axis. The main difference between these figures and Figure  3 is that we plot Equations (3) and (5), which give the average RHK at fixed UV − V rather than the average UV − V at fixed RHK.

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