Abstract:
We present the results of an Her emission line observational study of a sample of 75 pre-main sequence stars consisting of 17 HAEBE, 47 CTT and 11 WTT stars. Approximately half of the stars are faint, with a brightness in the V band greater than or similar to 13. The spectra have been taken at resolutions approximate to 30 km s(-1) and approximate to 80 km s(-1). The data shown provide information on equivalent width, radial velocity, variability and line profile.