  The SHALON atmospheric Cherenkov telescope has detected very high energy
gamma-ray emission at TeV energies from eight red dwarfs, namely, V388 Cas,
V547 Cas, V780 Tau, V962 Tau, V1589 Cyg, GJ 1078, GJ 3684 and GL 851.1.
Consequently, these red dwarfs have been suggested as sources of ultra-high
energy cosmic rays. In this work, we search for soft gamma-ray emission from
these TeV bright red dwarfs between 0.75-30 MeV using archival data from the
COMPTEL gamma-ray imaging telescope, as a follow-up to a similar search for GeV
gamma-ray emission using the Fermi-LAT telescope. Although, prima-facie, we
detect non-zero photon flux from three red dwarfs with high significance, these
signals can attributed to contamination from nearby sources such as Crab and
Cygnus, which are within the angular resolution of COMPTEL, and have been
previously detected as very bright point sources at MeV energies. Therefore, we
could not detect any statistically significant signal ($>3\sigma$) from any of
these eight red dwarfs from 0.75-30 MeV. We then report the 95% confidence
level upper limits on the differential photon flux (at 30 MeV), integral photon
flux and integral energy flux for all of the eight red dwarfs. The integral
energy flux limits range between $10^{-11}-10^{-10} \rm{ergs/cm^2/s}$.
