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The top documents tagged [galaxy density]
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galaxy density
HI Gas as Function of Environment When and where do galaxies stop accreting cool gas? How do they loose the cool gas? When do they stop forming stars?
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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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DESpec survey strategy : realistic mock catalogue and target selection
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DESpec survey strategy : realistic mock catalogue and target selection Stephanie Jouvel, Filipe Abdalla, Huan Lin, James Annis, Richard Kron 22 jun 2011.
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Topics in Astrophysics Michaelmas Term, 2010: Prof Craig Mackay
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MNRAS, submitted. Galaxy evolution Evolution in global properties reasonably well established What drives this evolution? How does it depend on environment?
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Newly Born Pulsars as Sources of High and Ultrahigh Energy Cosmic Rays Ke Fang University of Chicago ISCRA - Jul 9, 2012 1 KF, Kotera, Olinto 2012, ApJ,
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HI Gas as Function of Environment
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Newly Born Pulsars as Sources of High and Ultrahigh Energy Cosmic Rays
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Binary population synthesis implications for gravitational wave sources
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Pitch Angles of Clustered Spiral Galaxies in the Chandra Deep Field South Jazmin Berlanga Medina 1, Benjamin Davis 2, Daniel Kennefick 1,2 1 University.
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Strong Lensing Surveys and Statistics Dan Maoz. zqzq Survey strategies: Search among source population for lensed cases or Search behind potential lenses.
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