Brown dwarf discs
SEDs, Monochromatic Fluxes & Magnitudes
This page allows access to all the models currently available,
including those featured in Mayne and
Harries (2010) and Mayne, Harries and Rowe (in prep),
alongside current converged models.
If the Disc Mass is zero, the Disc Radius and Alpha are ignored.
At high inclinations stellar_direct fluxes are not sufficiently attenuated. All other SEDs are correct.
Physical propertiesPhysical properties of the system are tabulated at the bottom of the page, when they are available.
Mass: $mass Age: $age Period: $period Accretion: $accretion Areal: $areal Disc Mass: $dmass Disc radius: $radius Alpha: $alpha