Detection of Extended Red Emisson in the Diffuse Interstellar Medium

Extended Red Emission (ERE) has been detected in many dusty astrophysical objects and this raises the question: Is ERE present only in discrete objects or is it an observational feature of all dust, i.e. present in the diffuse interstellar medium? In order to answer this question, we determined the blue and red intensities of the radiation from the diffuse interstellar medium (ISM) and examined the red intensity for the presence of an excess above that expected for scattered light. The diffuse ISM blue and red intensities were obtained by subtracting the integrated star and galaxy intensities from the blue and red measurements made by the Imaging Photopolarimeter (IPP) aboard the Pioneer 10 and 11 spacecraft. The color of the diffuse ISM was found to be redder than the Pioneer intensities, contrary to that expected for scattered light (Diffuse Galactic Light [DGL]). The red DGL was calculated using the blue diffuse ISM intensities and the approximately invariant color of the DGL calculated with the DGL model. Subtracting the calculated red DGL from the red diffuse ISM intensities resulted in the detection of an excess red intensity. This represents the likely detection of ERE in the diffuse ISM since H-alpha emission cannot account for the strength of this excess and the only other known emission process applicable to the diffuse ISM is ERE. Thus, ERE appears to be a general characteristic of dust. From the correlation between N_HI and ERE intensity the ERE photon conversion efficiency was estimated at 10 +/- 3%