Astrocytes are known to play a key role in buffering extracellular pH variations and, in addition, they are particularly resistant to oxidative stress and subsequent lipid peroxidation. This great resistance may be ascribed to the presence of high concentrations of certain antioxidants, but another explanation may be the presence of a high quantity of plasmalogens, which are a special group of glycerophospholipids characterized by a vinyl ether bond instead of an ester bond in the sn-1 position of the glycerol backbone. Plasmalogens are sensitive to free radical attack and acidity, and numerous works have supported the hypothesis that they may be antioxidant molecules that protect cells from oxidative stress. The aim of this work was to investigate, on astrocytes in lactic acid-induced oxidative stress (pH 5.5), the behavior of phospholipids and, in particular, plasmalogens. Two main techniques, based on the susceptibility of the vinyl ether bond to hydrolysis, were employed in this study to measure plasmalogen levels. In both cases, the sn-1 vinyl ether linkage was cleaved using mercuric chloride, producing a lysophospholipid that was assessed by phosphorus measurement or using HCl treatment, producing a long-chain fatty aldehyde assayed by gas chromatography/mass spectrometry. On astrocytes in culture, only plasmenylethanolamine (PlmEtn) was evidenced, representing 40% of glycerophosphoethanolamine lipids. When astrocytes were incubated with lactic acid, no modification in the amount of PlmEtn was seen. Furthermore, free aldehydes and aldehydes corresponding to the quantity of intact plasmalogens were similar to those observed on controls. In addition, the constancy of two lipid peroxidation markers, thiobarbituric acid reactive substances and polyunsaturated fatty acids, was clear evidence of the resistance of these cells in lactic acid conditions. In conclusion, our results fail to demonstrate a major role of plasmalogens in the resistance of astrocytes in lactic acid-induced oxidative stress.