The observational result indicating a deficit in the frequency of
→ brown dwarf companions to Sun-like stars,
either relative to the frequency of less massive planetary companions or relative
to the frequency of more massive stellar companions.
However, this desert exists mainly for low-separation brown dwarfs detected
using orbital velocity surveys. No brown dwarf desert is noticed
at wide separations (J. E. Gizis et al. 2001, ApJ 551, L163).
See also: → brown; → dwarf;
→ desert.