  RAFGL2591 is a massive star-forming complex in the Cygnus-X region comprising
of a cluster of embedded protostars and young stellar objects located at a
distance of 3.33 kpc. We investigate low-frequency radio emission from the
protostellar jet associated with RAFGL2591 using the Giant Metrewave Radio
Telescope (GMRT) at 325, 610 and 1280 MHz. For the first time, we have detected
radio jet lobes in the E-W direction, labelled as GMRT-1 and GMRT-2. While
GMRT-1 displays a flat radio spectral index of $\alpha$ = -0.10 , GMRT-2 shows
a steeply negative value $\alpha$ = -0.62 suggestive of non-thermal emission.
H$_2$ emission maps show the presence of numerous knots, arcs and extended
emission towards the East-West jet, excited by the protostar VLA 3. In
addition, we report a few H$_2$ knots in the North-East and South-West for the
first time. The radio lobes (GMRT-1, GMRT-2) and H$_2$ emission towards this
region are understood in the context of the prominent East-West jet as well as
its lesser-known sibling jet in the North-East and South-West direction. To
model the radio emission from the lobes, we have employed a numerical model
including both thermal and non-thermal emission and found number densities
towards these lobes in the range 100 - 1000 cm$^{-3}$ . The misalignment of the
East-West jet lobes exhibits a reflection symmetry with a bending of $\sim$
20$\circ$ . We attempt to understand this misalignment through precession
caused by a binary partner and/or a supersonic side wind from source(s) in the
vicinity.
