Around HD 97300 and HD 97048 15 far-infrared sources are found. 3 of these are not included in the IRAS Point Source Catalogue, for 8 upper limits in the IPSC we have now determined fluxes, and confused sources have been separated better. This indicates that even this nearby region of star formation cannot be studied by just inspecting the IPSC. By including (V)JHK observations the bolometric luminosities of these sources are determined: they range from 02 to 20 LO. It concerns presumably
pre-main-sequence stars ranging in (expected) spectral type from M1 to A7.