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The top documents tagged [light ratios]
Signatures of Energy Injection in the CMB Rutgers University High Energy Theory Seminar 10/18/2011 Tracy Slatyer, Institute for Advanced Study based on
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Run your own GALEV model - an introduction
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© 2004 Pearson Education Inc., publishing as Addison-Wesley Dark Matter and the Fate of the Universe
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Sandage 1986 Roughly speaking, the Hubble sequence is also a sequence in star formation histories. HUBBLE TYPES and STAR_FORMATION HISTORIES
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1 Module 8: Clusters of Galaxies. General properties, masses and mass-to-light ratios, galaxy interactions, dynamic stability, the inter-galactic medium,
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Class 23 : The mass of galaxies and the need for dark matter How do you measure the mass of a galaxy? What is “dark matter” and why do we need it?
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Finsler Geometry vs. phenomenological anomaly in ultra-high energy and large scale CHANG Zhe Institute of High Energy Physics Chinese Academy of Sciences
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Luminosity Functions from the 6dFGS
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Dark Matter Searches in Space Xin Wu
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Heavy-to-light ratios as a test of medium-induced energy loss at RHIC and the LHC
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Optical Spectroscopy of Distant Red Galaxies Stijn Wuyts 1, Pieter van Dokkum 2 and Marijn Franx 1 1 Leiden Observatory, P.O. Box 9513, 2300RA Leiden,
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The Final (?) Frontier of Star and Planet Formation: Piled Deeper and Wider Michael R. Meyer
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