  Bow-shocks are produced in the local interstellar medium by the passage of
fast stars from the Galactic thin-disk and thick-disk populations with
velocities $V_* = $ 40-80 km/s. Stellar transits of local H I clouds occur
every 3500-7000 yr on average and last between $10^4$ and $10^5$ yr. There
could be 10-20 active bow shocks around low-mass stars inside clouds within
10-15 pc of the Sun. At local cloud distances of 3-10 pc, their turbulent wakes
have transverse radial extents $R_{\rm wake} \approx$ 10-300 AU, angular sizes
10-100 arcsec, and Lyman-alpha surface brightnesses of 2-8 Rayleighs in gas
with total hydrogen density $n_H \approx 0.1~{\rm cm}^{-3}$ and $V_* =$ 40-80
km/s. These transit wakes may cover an area fraction $f_A \approx (R_{\rm
wake}/R_{\rm cl}) \approx 10^{-3}$ of local H I clouds and be detectable in IR
(dust), UV (Lya, two-photon), or non-thermal radio emission. Turbulent heating
in these wakes could produce the observed elevated rotational populations of
H$_2$ ($J \geq 2$) and influence the endothermic formation of CH$^+$ in diffuse
interstellar gas at $T > 10^3$ K.
