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We present infrared and radio continuum observations of S 201 star formingregion. A massive star cluster is observed in this region, which containsdifferent classes of young stellar objects. The near-infrared colour-colour andcolour-magnitude diagrams are studied to discuss the nature of these sources.We have discovered the knots of molecular hydrogen emission at 2.122 micron inthe central region of S 201. These knots are clearly seen along the diffuseemission in north-west direction which are probably the obscured Herbig-Haroobjects. High sensitivity and high resolution radio continuum images from GMRTobservations at 610 and 1280 MHz show an interesting arc-shaped structure dueto the interaction between the H II region and the adjacent molecular cloud.The ionization front at the interface between the H II region and the molecularcloud is clearly seen by comparing the radio, molecular hydrogen and Br Gammaimages. The emission from the carriers of Unidentified Infrared Bands in themid-infrared 6-9 micron (possibly due to PAHs) as extracted from the MidcourseSpace Experiment survey (at 8, 12, 14 and 21 micron) is compared with the radioemission. The HIRES processed IRAS maps at 12, 25, 60, and 100 micron, havealso been used for comparison. The spatial distribution of the temperature andthe optical depth of the warm dust component around S 201 region, has beengenerated from the mid-infrared images.Comment: 13 pages, 27 figures in GIF & JPEG formats, Accepted for the  publication in Astronomy and Astrophysic

A study of the Galactic star forming region IRAS 02593+6016/S 201 in infrared and radio wavelengths