Passive disk
= Passive disk
= Passive disc
{synonym}
A passive <astrophysical disk> receives most of its heat from external irradiation rather than internal <viscous dissipation>. For a stellar disk, a rough criterion is $GM\dot M/R_*\ll L_*$. The actual local requirement compares absorbed stellar flux with viscous flux; incidence angle, shadowing and absorption can invalidate a luminosity comparison alone.