A&A 625, A101 (2019) Astronomy https://doi.org/10.1051/0004-6361/201834408 & © J. Bublitz et al. 2019 Astrophysics A new radio molecular line survey of planetary nebulae HNC/HCN as a diagnostic of ultraviolet irradiation J. Bublitz1,2, J. H. Kastner2, M. Santander-García3, V. Bujarrabal3, J. Alcolea3, and R. Montez Jr.4 1 Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, 38041 Grenoble, France 2 School of Physics & Astronomy, Center for Imaging Science, Laboratory for Multiwavelength Astrophysics, Rochester Institute of Technology, 54 Lomb Memorial Drive, Rochester, NY 14623, USA e-mail:
[email protected] 3 Observatorio Astronómico Nacional, Alfonso XII, 3, 28014 Madrid, Spain 4 Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138, USA Received 8 October 2018 / Accepted 7 April 2019 ABSTRACT Certain planetary nebulae (PNe) contain shells, filaments, or globules of cold gas and dust whose heating and chemistry are likely driven by UV and X-ray emission from their central stars and from wind-collision-generated shocks. We present the results of a survey of molecular line emission in the 88–236 GHz range from nine nearby (<1.5 kpc) planetary nebulae spanning a range of UV and X-ray luminosities, using the 30 m telescope of the Institut de Radioastronomie Millimétrique. Rotational transitions of thirteen molecules, including CO isotopologues and chemically important trace species, were observed and the results compared with and augmented by previous studies of molecular gas in PNe. Lines of the molecules HCO+, HNC, HCN, and CN, which were detected in most objects, represent new detections for four planetary nebulae in our study.