The following spectra were taken with the equipment described under “Spectroscopy”. Data were processed with MK32. Integration time was not more than a few minutes. Pixel dispersion ist 0.066 nm and spectral range is 50 nm for all spectra.
Full Width of Half Maximum (FWHM) was calculated for the H-Alpha line which gives a clue for the Doppler- and/or the pressure broadening. Further analysis with respect to the star’s parameters will follow soon...site still under construction.