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We present an atlas of high-S=N , high-resolution (v 6k m s 1 ) data of Be star emission and shell proles. We have collected proles of H and of Fe ii ,m ostly of the5317 transition. These lines have been selected to provide measures for the overall emission strength and for the velocity eld in these disks. We have collected data for 77 southern and equatorial programme stars, covering the period 1982-1993. This is the most comprehensive overview of prole shapes in Be disks. We propose a three-dimensional scheme in which most observed proles can be classied. The parameters are i) inclination, ii) optical depth, and iii) the pattern of the velocity eld. A search for short-term variability (timescales between ve days and a few minutes) in six stars ended with negative result. Shortest observed timescale for variability is a few days for well-developed disks in binary systems (HR 1910, HR 2142).

Atlas of high-resolution emission and shell lines in Be stars. Line profiles and short-term variability