These spectra have been taken with the Staranalyser which is a 100l/mm blazed grating available here. I used the Artemis 285 for most of the spectra which gave me a dispersion of about 11 Angstroms per pixel. Lines have been identified where possible.
|Spectrum of Vega used to for calibration purposes. The prominent hydrogen Balmer lines in A-type stars provide a good reference to calibrate your spectra.|
|Wolf-Rayet stars are excellent targets for spectroscopy even at low resolution. Their prominent emission lines due to the outflow of material from the star stand out clearly.|
Betelgeuse Antares Aldebaran Gamma Cygni