Abstract We present a grid of thermal emission contribution functions and their corresponding atmospheric spectra model for cloudy and cloud-free brown dwarfs, spanning effective temperatures T eff ∈ [500, 2000][K], surface gravities log g = [ 3.5 , 5.5 ] [cgs], sedimentation efficiencies f sed = 1, 2, 3, 4, and 8, and...
Myrla Phillippe, Theodora Karalidi, Elena Manjavacas et al.· The Astrophysical Journal· 0 citations
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