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The top documents tagged [balmer lines]
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balmer lines
13 March 201313rd MAXI Symposium Be Be. Talk Outline 1.Introduction to Be stars 2.Decretion vs. accretion 3.Interactions in binaries 4.Concluding remarks.
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Consequencies of the new intensity formula in many optical spectroscopy fields
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Lecture I: Introduction to White Dwarfs S. R. Kulkarni, E. Ofek srk/ay125
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Kirchhoff's laws,there are three types of spectra: continuum, emission line, and absorption line. High pressure, high temperature gas Low pressure,
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The Size, Structure & Ionization of the Broad-Line Region in NGC 3227 and NGC 4051 Nick Devereux (ERAU) Emily Heaton (ERAU) May 22 nd, 2013 Naples, Italy.
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Understanding Atoms Chapter 42. The Bohr Model – good but not perfect! For Hydrogen and “Hydrogenic” atoms predicts the Rydberg formula For Hydrogen.
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Chapter 13 Cont’d – Pressure Effects More curves of growth How does the COG depend on excitation potential, ionization potential, atmospheric parameters.
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First Spectroscopic Evidence for High Ionization State and Low Oxygen Abundance in Lyα Emitters ( arXiv:1208.3260, ApJ submitted ) subaru UM @NAOJ on 16/Jan/2013.
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1 Black Hole Masses from Reverberation Mapping Bradley M. Peterson The Ohio State University Collaborators: M. Bentz, S. Collin, K. Dasyra, K. Denney,
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Chapter 25: Quasars and active galaxies Features of quasars Quasars and distant galaxies Seyfert and radio galaxies Active galactic nuclei Supermassive.
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Lecture 2. Examination The course is assessed in three parts: Problem sets. The problem sets and the peer reviews. One of the sets will randomly be corrected.
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FFS at JET/Ameigs 02-09-13 FFS model Coupling Balmer positions to D10-2 thru Rydberg formula Coupling Lorentzian widths to the Griem Stark broadening formula.
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