ASTROPHYSICS AND SPACE SCIENCE, sa.1-2, ss.191-203, 1994 (SCI-Expanded)
V 923 Aql is one of the candidate B-e stars to be a binary star. In this research, optical and near-infrared spectral measurements of V 923 Aql is presented. V 923 Aql presents variable H Balmer line profiles with shell components. H alpha profiles present R/V, E/C and radial velocity variation. Shell parameters of the envelope are calculated.