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The top documents tagged [galaxy structure]
COSMIC MAGNETIC FIELDS ElisaBete M. de Gouveia Dal Pino IAG-USP UFRRJ, October 2005
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To measure the brightness distribution of galaxies, we must determine the surface brightness of the resolved galaxy. Surface brightness = magnitude within
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Black Hole in M83 Topic: Black holes Concepts: multi-wavelength observations, black hole evolution Missions: Hubble, Chandra, Swift Coordinated by the
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The Hubble Space Telescope Treasury Coma Cluster Survey Introduction, initial results, and future plans David Carter (Liverpool John Moores University)
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March 17, 2004STScI Colloquium1 ACS Observations of Distant Clusters of Galaxies & Protoclusters: New Constraints on Cluster and Galaxy Formation & Evolution
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Talk Outline
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The Distribution of Baryons in Galaxy Clusters and Groups Anthony Gonzalez University of Florida Dennis Zaritsky, Ann Zabludoff University of Arizona Ohio
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The Distribution of Baryons in Galaxy Clusters and Groups
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Physics Beyond the Standard Model David Toback Texas A&M University For the
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Black Hole in M83
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The Hubble Space Telescope Treasury Coma Cluster Survey
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Astronomy outreach at IGN Yebes Observatory: SPIDER
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