Possible astronomical sources of ultraviolet circularly polarized light(UVCPL) which might be responsible for enantiomeric selection in interstellarorganic molecules are considered, Synchrotron radiation from magnetic neutronstars has been suggested as a possible source of UVCPL. However, synchrotronradiation in these situations is not predicted to be strongly circularlypolarized. Very few such sources show optical synchrotron radiation and in thefew that do circular polarization has not been observed. Magnetic white dwarfsand white dwarf binaries (Polars) can be highly circularly polarized but anyeffect on molecular clouds and star formation regions must rely on rare chance encounters. Recent observations show that substantial levels of circularpolarization are present in reflection nebulae in star formation regions. Thismechanism produces polarized light exactly when and where it is needed inregions where star formation is occurring and organic molecules are known to be present.