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We present [Fe II] 1.64 {\mu}m imaging observations for jets and outflowsfrom young stellar objects (YSOs) over the northern part (~ 24'x45') of theCarina Nebula, a massive star forming region. The observations were performedwith IRIS2 of Anglo-Australian Telescope and the seeing was ~1.5"+-0.5". Elevenjet and outflow features are detected at eight different regions, and are namedas Ionized Fe Objects (IFOs). One Herbig-Haro object candidate missed in HubbleSpace Telescope H{\alpha} observations is newly identified as HHc-16, referringour [Fe II] images. IFOs have knotty or longish shapes, and the detection rateof IFOs against previously identified YSOs is 1.4 %, which should be treated asa lower limit. Four IFOs show an anti-correlated peak intensities in [Fe II]and H{\alpha}, where the ratio I([Fe II])/I(H{\alpha}) is higher for longishIFOs than for knotty IFOs. We estimate the outflow mass loss rate from the [FeII] flux, using two different methods. The jet-driving objects are identifiedfor three IFOs (IFO-2, -4, and -7), for which we study the relations betweenthe outflow mass loss rate and the YSO physical parameters from the radiativetransfer model fitting. The ratios of the outflow mass loss rate over the diskaccretion rate are consistent for IFO-4 and -7 with the previously reportedvalues (10^-2-10^+1), while it is higher for IFO-2. This excess may be from theunderestimation of the disk accretion rate. The jet-driving objects are likelyto be low- or intermediate-mass stars. Other YSO physical parameters, such asluminosity and age, show reasonable relations or trends.

[Fe II] 1.64 um Features of Jets and Outflows from Young Stellar Objects in the Carina Nebula