We present high-resolution (R D 1500È2000) spectra of the 4.27 km asymmetric stretching feature of solid in eight lines of sight observed with the Short Wavelength Spectrometer of the Infrared Space CO 2 Observatory. Two of the sources are Ðeld stars located behind the Taurus molecular cloud ; the others are young stellar objects (YSOs) of predominantly low-to-intermediate mass. We Ðnd a signiÐcant source-tosource variation in the solid abundance ratio in our sample : two lines of sight, Elias 18 andabundances of D 34%È37%, considerably higher than in other lines of sight CO 2 studied to date. In agreement with a previous study of Elias 16, we conÐrm a substantial (D20%) abundance of solid relative to in the quiescent intracloud medium. We compare the proÐles CO 2 H 2 O C O 2 with laboratory spectra of interstellar ice analogs from the Leiden Observatory Laboratory database. Results show that the 4.27 km proÐles toward Ðeld stars and embedded low-mass objects are remarkably similar to each other and seem to originate mostly in cold ice. In two higher mass YSOs H 2 O-rich (RAFGL 989 and S255 IRS1), the proÐles are clearly di †erent, and at least the latter source shows signs of thermal processing.