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Optimum damping on both channels is achieved by symmetrically winding the low-mass armature.
One contribution to the DIS g * p total cross section is the electroproduction of low mass vector mesons.
It is also extremely nimble, stopping and starting on a dime thanks to the low-mass platter.
Material of low mass per unit area and high surface porosity will tend not to reflect sound.
Both high and low mass protostars often possess powerful jets and outflows.