Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Maryland
University of Maryland at College Park
U. Maryland
University of Maryland, Department of Astronomy, College Park, MD 20742 University, College Park
University of Oxford
Blackett Laboratory, Imperial College, London, SW7 2BZ, UK
Blackett Laboratory, Imperial College of Science, Technology and Medicine, Prince Consort Street, London SW7 2BZ, UK.
Imperial College of Science and Technology, London, England
Blackett Laboratory, Imperial College, London SW7 2AZ
Imperial College, London, England, UK
Mullard Radio Astronomy Observatory, Cambridge, England
Science Research Council, Rutherford and Appleton Laboratories, Didcot, Oxon, England
Blackett Laboratory, Imperial College, London SW7 2BZ
Imperial College of Science, Technology, and Medicine, London, England
Blackett Laboratory, Imperial College, London, SW7 2BZ
Department of Physics, Imperial College, London SW7 2BZ, UK
Blackett Laboratory, Imperial College, London SW7 2BZ, UK
Department of Physics, University of Oxford, Parks Road, Oxford OX1 3PU, UK
Clarendon Laboratory, University of Oxford, Parks Road, Oxford OX1 3PU
Clarendon Laboratory, University of Oxford, Parks Road, Oxford OX1 3PU UK; STFC Rutherford Appleton Laboratory, Didcot, Oxfordshire OX11 0QX UK Laboratory, Imperial College, London SW7 2AZ, UK
University of Oxford, United Kingdom
University of Maryland
Univ. of Maryland
NSF, Washington, D.C.
Maryland, University, College Park, MD
Maryland, University, College Park, Md.
Astronomy Program, University of Maryland
Victoria, University, Canada
NSF, Washington, DC
NASA, Goddard Space Flight Center, Laboratory for Astronomy and Solar Physics, Greenbelt, Md.
Oklahoma, University, Norman, Okla.
Maryland Univ., College Park
STScI
Department of Astronomy, University of Maryland, 20742-2421, C
2D-FRUTTI Spectroscopy of 47-TUCANAE Subgiants
A Comment on the Metal Abundance of the Globular Cluster M71
A comment on the metal abundance of the globular cluster M71
A Comment on the Metal Abundance of the LMC Cluster NGC 2209
A Comparison Between Observed and Calculated IRAS Fluxes of G and K Giant Stars
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Profile ID: LFWR-SCP-P-130045