We will discuss the kinematics of halo gas in Milky Way analogs at redshift
0.2 based on new Keck LRIS spectroscopy of background quasars. The Doppler
shifts of the low-ionization-state gas are smaller than expected for gas in
virial equilibrium. The line profiles of the MgII absorption show
asymmetric shapes, and the Doppler shifts of the line wings have the same
sign of rotation as each star-forming disk. The total velocity width
spanned by each absorption line is a challenge to explain with simple
models. The observed line width can typically explain by adding a radial
inflow component in the disk plane to a rotating disk model.