Figure 10 from BOSS ULTRACOOL DWARFS. I. COLORS AND MAGNETIC ACTIVITY OF M AND L DWARFS

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BOSS ULTRACOOL DWARFS. I. COLORS AND MAGNETIC ACTIVITY OF M AND L DWARFS

Authors: Sarah J. Schmidt, Suzanne L. Hawley, Andrew A. West, John J. Bochanski, James R. A. Davenport, Jian Ge , and Donald P. Schneider

2015 The Astronomical Journal 149 158.

Provider: AAS Journals

Caption: Figure 10.

For each photosphere ﹩{{T}_{{\rm eff}}}﹩, log(﹩{{L}_{{\rm H}\alpha }}/{{L}_{{\rm bol}}}﹩) is shown as a function of chromosphere break for a range of chromospheric filling factors (colors given in the bottom right). The uncertainties in log(﹩{{L}_{{\rm H}\alpha }}/{{L}_{{\rm bol}}}﹩) are based on varying ﹩{{T}_{{\rm eff}}}﹩ by ±200 K, as discussed in the Appendix.

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