  We report detection of a Young Stellar Object with an evidence for an outflow
in the form of knots in the molecular hydrogen emission line (2.121 micron)
towards the massive star forming region IRAS 06061+2151. Near-infrared images
reveal IRAS 06061+2151 to be a cluster of at least five sources, four of which
seem to be early B type young stellar objects, in a region of 12 arcsec
surrounded by a nebulosity. The presence of the knots that are probably similar
to the HH objects in the optical wavelengths, suggests emerging jets from one
of the cluster members. These jets appear to excite a pair of knot-like objects
(Knot-NW and Knot-SE) and extend over a projected size of 0.5pc. The driving
source for the jets is traced back to a member of the cluster whose position in
the H-Ks/J-H color-color diagram indicates that it is a Class 1 type
pre-mainsequence star. We also obtained K band spectra of the brightest source
in the cluster and of the nearby nebular matter. The spectra show molecular
hydrogen emission lines but do not show Brackett gamma line at 2.167 micron.
These spectra suggest that the excitation of the molecular hydrogen lines is
probably due to a mild shock.
