New evidence for a substellar luminosity problem: Dynamical mass for the brown dwarf binary gl 417BC
We present new evidence for a problem with cooling rates predicted by substellar evolutionary models that implies that model-derived masses in the literature for brown dwarfs and directly imaged planets may be too high. Based on our dynamical mass for Gl
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Dupuy_New_evidence_for_a_substellar_2014.pdf||688.42 kB||Adobe PDF||Request a copy|
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