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The L to T Dwarf Transition
M. S. Marley, M. C. Cushing, D. Saumon
While the precise mechanism responsible for the L to T dwarf transition remains unclear, it is clearly caused by changing cloud characteristics. Here we briefly review data relevan…
Spitzer Infrared Spectrograph Observations of M, L, and T Dwarfs
T. L. Roellig, J. E. Van Cleve, G. C. Sloan +8
We present the first mid-infrared spectra of brown dwarfs, together with observations of a low-mass star. Our targets are the M3.5 dwarf GJ 1001A, the L8 dwarf DENIS-P J0255-4700,…
Shock Compression of Deuterium and the Interiors of Jupiter and Saturn
D. Saumon, T. Guillot
Recently, deuterium has been the focus of a high level of experimental and theoretical activity that was sparked by a disagreement on the experimental value of the maximum compress…
Radiative transfer in the refractive atmospheres of very cool white dwarfs
P. M. Kowalski, D. Saumon
We consider the problem of radiative transfer in stellar atmospheres where the index of refraction departs from unity and is a function of density and temperature. We present modif…