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 Encrenaz8, Margaret A. Frerking9, Paul Hartogh10, Wing-Huen Ip11, Michael A Janssen3, Christopher Jarchow12, Stephen Joseph Keihm13, Seungwon Lee9, Emmanuel Lellouch14, Cedric Leyrat15, Ladislav Rezac16, F. Peter Schloerb17 and Thomas R Spilker18, (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)Paris Observatory-PSL, LIRA, Meudon, France, (9)Jet Propulsion Laboratory, Pasadena, CA, United States, (10)Max Planck Institute for Solar System Research, Göttingen, Germany, (11)NCU National Central University of Taiwan, Jhongli, Taiwan, (12)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (13)JPL/NASA/Caltech, Pasadena, CA, United States, (14)LESIA, Observatoire de Paris, Paris, France, (15)Paris Observatory Meudon, Meudon, France, (16)Max Planck Institute for Solar System Research, Gottingen, Germany, (17)University of Massachusetts Amherst, Amherst, MA, United States, (18)Solar System Science and Exploration, Monrovia, CA, United States