Star formation in the Sh 2-53 region influenced by accreting molecular filaments

T. Baug, L. K. Dewangan, D. K. Ojha +6

We present a multi-wavelength analysis of a $\sim$30${}^{\prime }\times$30${}^{\prime }$ area around the Sh 2-53 region (hereafter S53 complex), which is associated with at least three H II regions, tw…