SIMBAD references

We analyzed the spectra of a well known SB1 binary HD199892 for which the projected rotational velocity v sin i, introduced in the literature, significantly differs when determined from the lines of Ca II at 3933 A and of Mg II at 4481 A. Contrary to the former findings, we discovered the signs of spectral lines of a companion star in the profile of H-beta as well as weak metallic lines in the high resolution high S/N spectra covering the most of the visual region. We estimated the secondary star to be a main sequence A4V star with a mass of 2.2 solar and derived its radial velocity which resulted in the mass of the primary M = 4.6 solar. Short sections of the spectra in the Mg II 4481 A and Ca II 3933 A regions are analyzed as well.