Post-CE states for originally 1.33 M_☉ NSs involved in interactions with wide variety of companions. Companions range in pre-CE mass from 12–20 M_☉, in radius from 100–1100 R_☉, and have convective envelopes. CE events initiated with smaller radius companions than those plotted (for a given mass) result in merger rather than envelope ejection. All evolutions computed result in NSs surviving CE, with none expected to undergo accretion-induced collapse to a BH. NSs generally gain more mass in interactions with more massive companions, but very extended radius at the onset of CE can lead to less mass accumulation. To compute the right-hand axis, we assume material is accreted from a Keplerian disk, and that adopt median NS properties of M_NS ≈ 1.39 M_☉, R_NS = 12 km. NSs undergoing these CE episodes survive to find themselves in close partnerships with helium-rich companions and orbital periods ranging from hours to days.