100+ Qso agn PowerPoint (PPT) Presentations, Qso agn PPTs

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Qingjuan Yu UC Berkeley April 21, 2006

Evolution of Accretion Disks around Massive Black Holes: Constraints from the Demography of Active Galactic Nuclei. Qingjuan Yu UC Berkeley April 21, 2006. (2005, ApJ, 634, 901, Qingjuan Yu, Youjun Lu, & Guinevere Kauffmann). (Tremaine et al. 2002). NGC 4258. Galactic center.

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293 views • 20 slides

Galaxy and Quasar Clustering at z=1

Galaxy and Quasar Clustering at z=1. Alison Coil University of Arizona. April 2007. Large-Scale Structure. SDSS :. Why do galaxies cluster? initial fluctuations in early universe gravity cosmology physics: galaxy formation Why high redshift? time leverage

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360 views • 20 slides

Properties of the point-like sources in the XMM-LSS field

Properties of the point-like sources in the XMM-LSS field. Olga Melnyk and XMM-LSS collaboration N. Clerc, L. Chiappetti, A. Elyiv, P.Gandhi, E.Gosset, M. Pierre, M. Plionis, T.Sadibekova, M.Salvato, P.-G. Sprimont, J.Surdej. Software Clusters of galaxies Sacley team. Spectroscopy

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282 views • 20 slides

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Qso agn - PowerPoint PPT Presentation

Qingjuan Yu UC Berkeley April 21, 2006

Galaxy and Quasar Clustering at z=1

Properties of the point-like sources in the XMM-LSS field