Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Lund Observatory
Lund Observatory, Sweden
HST Eta Carinae Treasury Project Team
Lund Observatory, Lund University, PO Box 43, 22100 Lund, Sweden Lund
Lund Observatory, University of Lund, Sweden
Lund Observatory, Lund University, Sweden
Lunds Universitet, Lund, Sweden
Lund, Universitet, Lund, Sweden
Department of Physics, Lund University, PO Box 118, 22100 Lund, Sweden
Atomic Astrophysics, Lund Observatory, Box 43, 221 00 Lund, Sweden
Atomic Astrophysics, Lund Observatory, Lund University, Box 43, 221 00 Lund, Sweden
Atomic Astrophysics, Lund Observatory, Lund University, Box 43, SE-221 00 Lund, Sweden
Lund Observatory, Lund University, P. O. Box 43, Lund, 221 00, Sweden
Lund Observatory, Lund University, PO Box 43, 22100 Lund, Sweden Astrophysics, Lund Observatory, Lund University, PO Box 43, 22100 Lund, Sweden Astrophysics, Department of Astronomy, Lund University, PO Box 43, 22100 Lund, Sweden of Physics, Lund University, PO Box 118, 22100 Lund, Sweden Department, Lund University, S-22100 Lund, Sweden
Lund Obs.
Department of Physics, University of Lund, Box 118, 221 00 Lund, Sweden; Lund Observatory, Lund University, Box 43, 221 00 Lund, Sweden. Spectroscopy, Department of Physics, University of Lund, Box 118, 221 00 Lund, Sweden
Atomic Astrophysics, Lund Observatory, Lund University, Box 43, 22100, Lund, Sweden
Lund Observatory, Lund University, P.O. Box 43, 221 00 Lund, Sweden
Lund Observatory, Lund University, P.O. Box 43, S-221 00 Lund, Sweden Spectroscopy, Department of Physics, University of Lund, Sölvegatan 14, S-223 62 Lund, Sweden Astrophysics, Lund Observatory, Lund University, Box 43, SE-22100 Lund, Sweden
University of Lund, L
A glimpse into the post-COSTAR GHRS: detections of As II and Bi II in the UV spectrum of the HgMn star χ Lupi.
A model for the origin of the anomalous and very bright UV lines of Fe II in gaseous condensations of the star η Carinae
A New Multiplet Table for Fe
A new multiplet table for Fe I
A Radiative Cycle with Stimulated Emission from Atoms (Ions) in an astrophysical Plasma
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Profile ID: LFWR-SCP-P-118150