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The top documents tagged [line profiles]
Singapore Air Final
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Line Profiles Note - Figure obtained from lsa.atnos/SAElp05.htmlsa.atnos/SAElp05.htm
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Grop 9 Magnetics_powerpoint2015 Updated 17 4 15
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Science With the Extreme-ultraviolet Spectrometer (EIS) on Solar-B by G. A. Doschek (with contributions from Harry Warren) presented at the STEREO/Solar-B
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Possible disk emission in the BLR of AGN Edi Bon Astronomical Observatory Belgrade, Serbia
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L. Č. Popović 1, D. Ilić 2 1- Astronomical
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Astrophysics Yr 2 Session 6 Astronomical Spectroscopy
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Emission mechanisms. II GiorgioMatt Giorgio Matt (Dipartimento di Fisica, Università Roma Tre, Italy) Reference: Rybicki & Lightman, “Radiative processes
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High resolution (sub)millimetre studies of the chemistry of low-mass protostars Jes Jørgensen (CfA) Fredrik Schöier (Stockholm), Ewine van Dishoeck (Leiden),
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Are inputs to standard solar models correct? OR The problem with solar abundances Sarbani Basu Yale Univesity
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1 Atmospheric dynamics of red supergiant stars Andrea Chiavassa Groupe de Recherche en Astronomie et Astrophysique du Languedoc GRAAL Thesis advisor: Bertrand
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Line Profiles of Magnetically Confined Winds Stephanie Tonnesen Swarthmore College
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Black Hole Physics with Constellation-X Chris Reynolds Department of Astronomy University of Maryland College Park
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