Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
UCL
University College London;
University College London UK
Department of Physics and Astronomy, University College London
University College London, UK
Univ. College London
University College London, London, UK
Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, UK
University College London, Department of Physics and Astronomy, Gower St., London WC1E 6BT, UK
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT
Joint Institute for Laboratory Astrophysics, Boulder, CO; University College, London, England
California, University, Berkeley, Calif; Sussex, University, Brighton, England
University College, London
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK
University Coll., London, UK
Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
University of Sussex, UK
Department of Physics and Astronomy, University College London, Gower Street, London WC1E6BT, UK
University College London, United Kingdom
University of California, Berkeley, California, US
U. College London
Physics and Astronomy Department, University College London
Department of Physics and Astronomy, University College London, Gower Street, London WC1E6BT
Sussex, University, Brighton, England; Joint Institute for Laboratory Astrophysics, Boulder, Colo.
Istituto di Fisica dello Spazio Interplanetario CNR - Roma, Italy
Department of Physics and Astronomy, University College, Gower Street, London, WC1E 6BT
University College, London, UK
Maryland, University, College Park
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK.
University College, London, United Kingdom
Department of Physics and Astronomy, University College London, UK
Department of Physics and Astronomy, University Co
"PAH" emission bands in selected planetary nebulae: a study of the behaviour with gas phase C/O ratio
2.4 - 197 micron spectroscopy of OH/IR stars: The IR characteristics of circumstellar dust in O-rich environments
3D Photoionisation Modelling of NGC 6302
8-13 micron spectra of very late type Wolf-Rayet stars
870 um observations of evolved stars with LABOCA
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Profile ID: LFWR-SCP-P-25747