Abstract:The authors have identified two new possible planetary nebulae using the Parker, Gull, and Kirshner (1979) emission-line survey of the galactic plane. Both objects exhibit very strong [O III] λ5007 li...The authors have identified two new possible planetary nebulae using the Parker, Gull, and Kirshner (1979) emission-line survey of the galactic plane. Both objects exhibit very strong [O III] λ5007 line emission, a symmetrical morphology, and a faint blue central star.Read More