Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Aarhus
Bristol, University, Bristol, England
Institute of Physics and Astronomy, University of Aarhus, DK-8000, Aarhus C, Denmark
University of Bristol, Bristol, UK
Institute of Physics and Astronomy, University of Aarhus, DK-8000, Aarhus, Denmark
School of Chemistry, The University, Bristol BS8 1TS.
Bristol, University, England
Observatoire de Meudon, France
Department of Physics and Astronomy, University of Aarhus, 8000 Aarhus C, Denmark
Department of Physics and Astronomy, Århus University, 8000 Århus C, Denmark
Institute of Physics and Astronomy, University of Århus, Ny Munkegade, DK-8000 Århus C, Denmark
School of Chemistry, University of Bristol, Cantock's Close, Bristol BS8 1TS, UK
Institute for Storage Ring Facilities, University of Aarhus, 8000 Aarhus C, Denmark of Chemistry, University of Bristol, Bristol BS8 1TS
Institute of Physics and Astronomy, University of Aarhus, DK-8000, Aarhus C, Denmark and University of Bristol, School of Chemistry, Cantock's Close, Bristol BS8 1TS, UK
Observatoire de Paris-Meudon, LERMA and UMR 8112 of the CNRS, 92195 Meudon Principal Cedex, France; Université de Cergy-Pontoise, LERMA and UMR 8112 of the CNRS, 95806 Cergy Cedex, France
School of Chemistry, Cantock's Close, University of Bristol, Bristol BS8 1TS, UK
Department of Geology, University of Nottingham, Nottingham NG7 2RD England
Department of Physics and Astronomy, Aarhus University, Denmark.
School of Chemistry, University of Bristol, Bristol BS8 1TS, UK
Institute of Physics and Astronomy, University of Aarhus, DK-8000 Aarhus C, Denmark
School of Chemistry, University of Bristol
Institute of physics and Astronomy, University of Aarhus, 8000 Aarhus c, Denmark
Bristol Univ., United Kingdom
Institute for Storage Ring Facilities, University of Aarhus, DK-
3D model of bow shocks
A 3D view of the outflow in the Orion Molecular Cloud 1 (OMC-1)
A method for detection of structure
A model for OH masers in star-forming regions
A Model for the Variability of SIO Masers in Mira Variables
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