X3: A High-mass Young Stellar Object Close to the Supermassive Black Hole Sgr A*

To date, the proposed observation of Young Stellar Objects (YSOs) in Galactic center (GC) still raises question where and how these objects could have formed due to violent vicinity Sgr~A*. Here, we report multi-wavelength detection a highly dynamic YSO close Sgr~A* that might be member IRS13 cluster. We observe beforehand known coreless bow-shock source X3 near- mid-infrared (NIR/MIR) with SINFONI (VLT), NACO ISAAC VISIR SHARP (NTT), NIRCAM2 (KECK). In radio domain, use CO continuum H30$\alpha$ ALMA observations identify system components at different temperatures locations concerning central stellar source. It is suggested radio/submm combination NIR Br$\gamma$ line can associated protoplanetary disk which consistent manifold reveal complex molecules elements such as PAH, SIV, NeII ArIII dense compact region. Based on photometric analysis, infer mass $15^{+10}_{-5} M_{\odot}$ for related age few $10^4$ yr. Due this estimate required relaxation time scales high-mass stars, finding an indication ongoing star formation inner parsec. The proper motion 3d distance imply relation IRS13. argue may serve birthplace young stars are ejected evaporation