Young open clusters (age ≤10 Myr) are idiosyncratic to study star formation in our galaxy. It is important to study the properties of young open clusters to understand how star formation takes place in both local and Galactic plane scales. Moreover, one of the important questions in the field of star formation is the role of stellar feedback on the subsequent star formation processes. In the present study to understand star formation we performed the multiwavelength analysis of open star cluster Waterloo 01 and an HII region Sh 2-208. We found that both regions have massive OB-type stars as member stars and the Sh 2-208 region encompasses an infra-red cluster [BDS2003]64. Both regions have elongated morphology and are placed at a distance of 3.53 kpc with reddening of 0.83 mag and 0.65 mag respectively. Radio continuum emission, distribution of warm and cold dust emission, molecular morphology, and various feedback pressures profoundly signify that massive stars present at the center of Waterloo 01 cluster affect its surrounding environment and generate an HII region Sh 2-208. Massive stars present in this region also affect its environment and further star formation is going on at the place of Sh 2-208. Hence, we identified feedback loops of star formation in these regions.
