Spectral study of V565 Mon: probable FU Ori-like or chemically peculiar star

We present the detailed spectroscopic study of V565 Mon pre-main-sequence star, which is illuminating star Parsamian 17 cometary nebula. Observations were performed with 2.6 m telescope in Byurakan Astrophysical Observatory 15 February 2018. Radial velocities and equivalent widths most prominent lines are presented. built spectral energy distribution estimated main parameters for example obtained bolometric luminosity $L_{V565}\approx 130L_{\odot} $ . Considering all features we came to conclusion that this young intermediate-mass can belongs some intermediate class between T Tau HAeBe stars. Very unusual a presence strong absorption Ba II spectrum. Possible explanations on issue discussed. Hence, think unique example, help understand open questions nucleosynthesis problem