Well, red dwarfs are stars too.
I found this online:
Note that the multiplicity rate, or the probability that a given
system has more than one component, is only 31%. The low rate is
because M-type dwarfs (also called red dwarfs) dominate the solar
neighborhood (a full 72% of the stellar sample, i.e. not L/T/P
objects, are M-type dwarfs), and do not have companions as often as
their more massive stellar cousins.
I found this online:
Note that the multiplicity rate, or the probability that a given
system has more than one component, is only 31%. The low rate is
because M-type dwarfs (also called red dwarfs) dominate the solar
neighborhood (a full 72% of the stellar sample, i.e. not L/T/P
objects, are M-type dwarfs), and do not have companions as often as
their more massive stellar cousins.