Protoclusters PowerPoint PPT Presentations
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3% baryon. Hubble constant:H0=73km /s /Mpc. Age of the universe: 13.7 Gyr ... Baryon density, b = 0.015h-1. Cosmological constant, 0 = 0.7 ...
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Coevolution of black holes and galaxies at high redshift David M Alexander (Durham)
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Controls the re-ionization of the Universe. Determines the phase structure of the Interstellar Medium ... Kurk, Pentericci, R ttgering, Miley & Heckman: ...
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... disk surrounding a SMBH = coeval SMBH galaxy formation? ... M-s relation coeval SMBH and galaxy formation? QSO dust heating: star formation or AGN? ...
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0. Introductory remarks about galaxy formation & evolution and why clusters ... for overdensities in galaxies (Miley, Rottgering, de Breuck, Kurk, Overzier) ...
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High Redshift Galaxies
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At z 2 all baryons are found in the Lya forest, but about 45% of the baryons z 2 ... Absorption lines in X-ray and UV quasar spectra ...
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That there is a connection is clear from the various correlations found between star ... Stars form in spiral arms. M33 Spitzer Image. From Verley et al. ...
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AGN Feedback deposits large amounts of energy influencing the evolution of ... (Overzier, Venemans, Kurk, Miley, de Breuk, van Breugel, Maschietto, van Breugel, ...
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Mark I and II imaging of Virgo galaxies. 18 nearby clusters: Solanes et al. 2001 ... this with large fraction of Virgo spirals with unusual Ha distributions? ...
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Overview and progress
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Roberto Soria (CfA) The Antennae, courtesy of G Fabbiano (CfA) ... Implications for SMBH growth at high z. Seed IMBHs from early nuclear starburst or from mergers? ...
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Search for a statistical description of the dark matter / galaxy distribution ... Based on GIF/VIRGO N-body. simulations by Jenkins et al. (1998) At z=3: r0~1 ...
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Star Formation at Very Low Metallicities
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... mechanism for ellipticals and bulges, which are collections of old ... Big question: what's the best way to constrain the baryonic physics of galaxy ...
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Michael Burton (UNSW), Maria Hunt (UNSW), Jim Caswell (ATNF) ... Minier, Purcell, Hill et al, 2004. Cold Core. Hot Molecular. Core. Ionized Core (UCHII region) ...
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Project Scientist LMT. Instituto Nacional de Astrofisica, Optica y Electronica ... Basic observational properties of the ISM and galaxies at FIR-mm wavelengths. ...
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Spinrag in het Heelal Door Joris Voorn The spiderweb galaxy: a forming massive cluster galaxy at z 2 (Miley et al. 2006) Opbouw Eigenschappen radiostelsel ...
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Robust identification of distant Compton-thick AGNs. IR AGN ... First insight into AGN activity in a Distant Protocluster. Lehmer, Alexander, et al., in prep ...
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There is a spectrum of density perturbations gravitational potential ... day L* galaxies; similar to big bulges and intermediate-luminosity Ellipticals ...
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A Brief Summary of Star Formation in the Milky Way Yancy L. Shirley Star Formation Disucssion Group April 1 2003 (no joke!) Outline Brief overview of Milky Way Star ...
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DEEP06 Oct 9 13, 2006 Sintra, Portugal. Isotropy of strong sources. DEEP06 Oct 9 13, 2006 Sintra, Portugal. Isotropy of faint sources ...
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Large 10-100 parsecs across (1014 1015 km) 1000X mass of our Sun ... bound, meaning they will exist as collection orbiting each other forever. ...
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Intermediate-Mass BHs and star clusters. Roberto Soria (CfA / University College London) ... old BHs, recycled systems? In globular. clusters? IMBH formation in ...
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G.K. Miley (Leiden),H.J.A.Rottgering (Leiden), J Kurk (MPIA) B.Venemans (IoA ... is several times higher than in the rest of the field (Miley et al, 06 in press) ...
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Direct observations of cluster galaxy progenitors forming at high redshift (z 2) ... galaxies brighter in the past (i.e., at higher z, M was brighter), but, Tinsley ...
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Tracey Hill1, Michael Burton1, Vincent Minier2, Mark Thompson3, Andrew Walsh1, ... Inset: An example SIMBA map: G10.15-0.34 with 1.2mm overlays. ...
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