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We present an analysis of the IRAS 08589-4714 star-forming region. Thisregion harbors candidate young stellar objects identified in the WISE andHerschel images using color index criteria and spectral energy distributions(SEDs). The SEDs of some of the infrared sources and the 70 microns radialintensity profile of the brightest source (IRS 1) are modeled from Herschelfluxes using the one-dimensional radiative transfer DUSTY code. For theseobjects, we estimate the envelope masses, sizes, densities, and luminositieswhich suggest that they are very young, massive and luminous objects at earlystages of the formation process. Color-color diagrams in the bands of WISE and2MASS are used to identify potential young objects in the region. Thoseidentified in the bands of WISE would be contaminated by the emission of PAHs.We use the emission distribution in the infrared at 70 and 160 microns, toestimate the dust temperature gradient. This suggests that the nearby massivestar-forming region RCW 38, located ~ 10 pc of the IRAS source position may becontributing to the photodissociation of the molecular gas and to the heatingof the interstellar dust in the environs of the IRAS source.

The IRAS 08589-4714 star-forming region