Image Details

Choose export citation format:

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 11.

Typical run of our Monte Carlo simulations in Section 4.1. The panel on the left shows the intrinsic color–color relation, without observational errors or selection effects, together with Equation (12), which we used to generate the data. The panel on the right shows the same sample, but with observational errors and flux limits applied, and a fit to the simulated data. On both panels red points are the most active stars, with log  RHK > −4.5, green points have −5.0 < log  RHK < −4.5, while blue points have log  RHK < −5.0. Equation (12) and our fit to the simulated data are plotted at the median log  RHK of each bin.

Other Images in This Article

Show More

Copyright and Terms & Conditions