We suggest that supersonic linewidths inferred from recent measurements of
magnetic fields toward the core position in dark interstellar molecular clo
uds may be due to transverse waves of magnetization propagating in a poorly
ionized, magnetically ordered gas-dust medium composed of tiny ferromagnet
ic dusty grains suspended in a cold gaseous cloud of molecular hydrogen. (C
) 2000 MAIK "Nauka/Interperiodica".