The Nucleus and Coma of Comet 67P/C-G at Millimeter and Submillimeter Wavelengths as seen by MIRO
Mark D Hofstadter1, Samuel Gulkis2, Mark Allen3, Paul Von Allmen3, Gerard Beaudin4, Nicolas Biver5, Dominique Bockelée-Morvan6, Mathieu Choukroun7, Jacques Crovisier5, Pierre Encrenaz4, Therese Encrenaz5, Margaret A. Frerking8, Paul Hartogh9, Wing-Huen Ip10, Michael A Janssen3, Christopher Jarchow11, Stephen Joseph Keihm12, Seungwon Lee8, Emmanuel Lellouch13, Cedric Leyrat14, Ladislav Rezac15, F. Peter Schloerb16 and Thomas R Spilker17, (1)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, CA, United States, (2)California Institute of Technology, Pasadena, CA, United States, (3)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (4)Observatoire de Paris, LERMA, Paris, France, (5)LESIA Observatoire de Paris, Meudon, France, (6)Paris Observatory, Paris, France, (7)Jet Propulsion Laboratory, Pasadena, United States, (8)Jet Propulsion Laboratory, Pasadena, CA, United States, (9)Max Planck Institute for Solar System Research, Göttingen, Germany, (10)NCU National Central University of Taiwan, Jhongli, Taiwan, (11)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (12)JPL/NASA/Caltech, Pasadena, CA, United States, (13)LESIA, Observatoire de Paris, Paris, France, (14)Paris Observatory Meudon, Meudon, France, (15)Max Planck Institute for Solar System Research, Gottingen, Germany, (16)University of Massachusetts Amherst, Amherst, MA, United States, (17)Solar System Science and Exploration, Monrovia, CA, United States
