Discovery of Four New Clusters in the Cygnus Cloud

We report the discovery of four new open clusters (named as QC 1, 2, QC3 and 4) in direction Cygnus Cloud select their members based on five astrometric parameters (l, b, \varpi, \mu^*_{\alpha}, \mu_{\delta}) Gaia DR2. also derive astrophysical for each cluster. Structure are generated by fitting radial density distribution with King's profile. Using solar metallicity, we performed isochrone-fitting purified color-magnitude diagrams (CMDs) to achieve age clusters. The known cluster NGC 7062 at adjacent area is chosen verify our identification process. estimated distance, reddening good agreement literature.