Extended Red Emission in the "Evil Eye" Galaxy (NGC4826)

We obtained low-resolution, long-slit 5300--9100 A spectroscopy of NGC4826 (a nearby galaxy with an absorbing dust lane (DL) asymmetrically placed across its bulge, associated with several HII regions) with a slit encompassing its bulge, positioned across its nucleus. The wavelength-dependent effects of absorption and scattering by dust in the lane are evident when comparing the observed stellar SEDs of pairs of positions symmetrically located with respect to the nucleus, one on the DL side and one on the opposite side of the bulge, by assuming that the intrinsic ISRF is axi-symmetric. We analyzed these SED ratios through the multiple-scattering radiative transfer model of Witt and Gordon and we discovered strong residual Extended Red Emission (ERE) from a region of the DL within a distance of 13 arcsec from the nucleus, adjacent to a broad, bright HII region. ERE is an established phenomenon in the literature interpreted as originating from photoluminescence by nanometer-sized clusters, illuminated by UV/optical photons. The complex radial variation of the ERE band-integrated intensity and of the ERE-to-scattered light band-integrated intensity ratio with the optical depth of the model derived for the DL and with the strength and hardness of the illuminating ISRF is reproduced consistently through the theoretical interpretation of the photophysics of the ERE carrier by Smith and Witt. When examined within the context of ERE observations in a variety of Galactic dusty environments (e.g. the diffuse ISM, reflection nebulae, planetary nebulae and the Orion Nebula), we conclude that the ERE photon conversion efficiency in NGC4826 is as high as found elsewhere, but that the size of the actively luminescing nanoparticles there is about twice as large as those thought to exist in the Galactic diffuse ISM.