[en] We report on a sample of 48 nearby, star-forming galaxies observed with the Cosmic Origin Spectrograph on the Hubble Space Telescope. We measure the kinematics of warm gas in galactic outflows using a combination of four Si ii absorption lines. We use multi-wavelength ancillary data to estimate stellar masses (M_*), star formation rates (SFR), circular velocities (v_circ), and morphologies. The galaxies cover four orders of magnitude in M_* and SFR, and sample a wide range of morphologies from starbursting mergers to normal star-forming galaxies. We derive 3.0–3.5σ relations between outflow velocity and SFR, M_*, and v_circ. The outflow velocities scale as SFR^0.08−0.22, $M_{\ast <!--\; ???\; -->}^{0.12-<!--\; ???\; -->0.20}$ and $v_{\mathrm{c}\mathrm{i}\mathrm{r}\mathrm{c}}^{0.44-<!--\; ???\; -->0.87},$ with the range depending on whether we use a maximum or a central velocity to quantify the outflow velocity. After accounting for their increased SFR, mergers drive 32% faster outflows than non-merging galaxies, with all of the highest velocity outflows arising from mergers. Low-mass galaxies (log(M_*/ M_⊙) < 10.5) lose some low-ionization gas through galactic outflows, while more massive galaxies retain all of their low-ionization gas, unless they undergo a merger.