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We report on diffraction-limited observations in the far-infrared and sub-millimeter of the Cluster B region of Serpens (G3-G6 Cluster) and of the HerbigBe star to the south, VV Ser. The observations were made with the Spitzer MIPSinstrument in fine-scale mode at 70um, in normal mapping mode at 160um (VV Seronly), and the CSO SHARC-II camera at 350um (Cluster B only). We use these datato define the spectral energy distributions of the tightly grouped members ofCluster B, many of whose SEDs peak in the far-infrared. We compare our resultsto those of the c2d survey of Serpens and to published models for thefar-infrared emission from VV Ser. We find that values of Lbol and Tbolcalculated with our new photometry show only modest changes from previousvalues, and that most source SED classifications remain unchanged.

Serpens Cluster B and VV Ser Observed With High Spatial Resolution at 70, 160, and 350um