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The top documents tagged [strongest lines]
Florin Garoi Programme for Research-Development-Innovation for Space Technology and Advanced Research - STAR Romanian Space Week, 12-16 May 2014, Bucharest,
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Stars were originally classified according to their spectra (strength = width of their absorption lines) either from a purely observational perspective
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Chandra Emission Line Diagnostics of Sco Carolin N Cardamone Advisor: David Cohen
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Spectral simulations of a H-C-O-Si plasma David Cohen with V. Swisher, M. Brown Swarthmore College Mar. 12, 2006 For the Plasma Dynamics Laboratory, University
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Binarity & Symbiotics Hugo E. Schwarz. Cerro Tololo Inter-American Observatory, NAOA/AURA
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July 11 X-Ray Gratings Workshop Capella Grating Data and the Emission Line Project - An Update Priya Desai (CfA) Nancy Brickhouse Jeremy Drake Dave Huenenmoerder
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Molecule Search: Summing Lines Demo: Detection of Isotopomers of HC 5 N In 39-48 GHz GBT Survey of TMC Glen Langston (NSF) + Many Students
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CHEMICAL ANALYSIS OF EXHALED HUMAN BREATH USING HIGH RESOLUTION MM-WAVE ROTATIONAL SPECTRA Tianle Guo, Jessica R. Thomas, Daniela R. Branco, Ivan R. Medvedev
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Protoplanetary disks as seen by the IRAM array Vincent Pietu (LAOG) A few important points in the observations and analysis related to the survey we have
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8. The Classification of Stellar Spectra Goals :
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Characteristics of Stars Chapter 3 Section 4 ISN p. 33
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