  We have obtained spectra of the reflection nebulosity illuminated by two
heavily embedded IRAS sources in the L1641 molecular cloud, Re 50 and IC 430
(V883 Ori). Examination of these spectra in combination with their other
properties indicates that these objects are FU Orionis objects. Our spectrum of
L1551 IRS 5 confirms the FU Ori classification made for this star by Mundt et
al. (1985).
