Estudio infrarrojo de los jets estelares MHO 2147/2148

In this contribution, we present an analysis of the stellar jets MHO 2147 and MHO 2148, located in the galactic plane, in the Ophiuchus region, at a distance of 3.23 kpc. They have been observed with GSAOIGeMS/GEMINI in the H (2.122 m) and K (2.2 m) bands and by the VVV VISTA survey in the J, H y K filters. We analyze the morphology of both jets, which are perpendicularly oriented. These jets show a chain of knots that delineate Sprofiles, suggesting the precession of the jet axis or the binarity of the exciting source.