Year: 2016
Type: article
Abstract: Context. The H i halo clouds of the Milky Way, and in particular the intermediate-velocity clouds (IVCs), are thought to be connected to Galactic fountain processes. Observations of fountain clouds are important for understanding the role of matter recycling and accretion onto the Galactic disk and subsequent star formation.
Source: Astronomy and Astrophysics
Authors: T. Röhser, J. Kerp, D. Lenz, B. Winkel
Institutions: University of Bonn, Max Planck Institute for Radio Astronomy
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Funders: National Aeronautics and Space Administration, UK Space Agency, International Max Planck Research School for Environmental, Cellular and Molecular Microbiology, European Space Agency, Science Foundation Ireland, Deutsche Forschungsgemeinschaft, Partnership for Advanced Computing in Europe AISBL, Centre National d’Etudes Spatiales, Tekes, Max-Planck-Gesellschaft, China Scholarship Council, Centre National de la Recherche Scientifique, Ministerio de Ciencia e Innovación, Ministério da Ciência, Tecnologia e Ensino Superior, International Max Planck Research School for Advanced Methods in Process and Systems Engineering, Science and Technology Facilities Council, Fundação para a Ciência e a Tecnologia, Institut National de Physique Nucléaire et de Physique des Particules
Awards: G4201897825, G7321284446
OpenAlex ID: W2521073679