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Francesco Damiani Young Clusters in the Gaia-ESO Survey, Palermo, 20 May 2014 Francesco Damiani INAF-Osservatorio Astronomico di Palermo, ITALY Stellar.
METO 621 Lesson 5. Natural broadening The line width (full width at half maximum) of the Lorentz profile is the damping parameter, . For an isolated.
R. K. Ulrich 1 · L. Bertello 1 · J. E. Boyden 1 · L. Webster 1 Interpretation of Solar Magnetic Field Strength Observations 1 Department of Physics and.
SPINOR Inversions based on RFs
Broad iron lines from accretion disks
S PECTRAL LINE ANALYSIS : LOG G Giovanni Catanzaro INAF - Osservatorio Astrofisico di Catania 9 april 2013 Spring School of Spectroscopic Data Analyses.
