Crater-related flow features on Ceres - Implications for cryovolcanism
Katrin Krohn1, Ralf Jaumann1, Katrin Stephan2, Katharina A. Otto3, Nico Schmedemann4, Roland J Wagner1, Klaus-Dieter Matz1, Federico Tosi5, Francesca Zambon5, Isabel von der Gathen1, Franziska Schulzeck1, Debra Buczkowski6, Harald Hiesinger7, Harry Y McSween Jr8, Carle M Pieters9, Frank Preusker1, Thomas Roatsch10, Carol A Raymond11, Christopher T Russell12 and David A Williams13, (1)German Aerospace Center DLR Berlin, Berlin, Germany, (2)German Aerospace Center, Berlin, Germany, (3)German Aerospace Centre (DLR), Berlin, Germany, (4)Free University of Berlin, Berlin, Germany, (5)INAF-IAPS, Rome, Italy, (6)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (7)University of Münster, Institute for Planetology, Münster, Germany, (8)University of Tennessee, Earth & Planetary Sciences, Knoxville, TN, United States, (9)Brown University, Earth, Environmental and Planetary Sciences, Providence, RI, United States, (10)German Aerospace Center (DLR), Berlin, Germany, (11)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (12)University of California, IGPP/EPSS, Los Angeles, CA, United States, (13)Arizona State University, Tempe, AZ, United States
