Recent Studies of the Spectrum of V1016 Cygni
Two coudé spectra of V1016 Cyg taken on June 24 and 27, 1979 were reduced, using a computer programme developed in Marseille, Radial velocities and full widths at half maximum were measured for the emission lines, and are summarized in the following table were VR is the mean radial velocity in km s−1, DV the velocity corresponding to the mean FWHM and Xi the effective ionization potential for the ion.
KeywordsEmission Line Molecular Band Symbiotic Star Mira Variable Line Equivalent Width
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