Title: Slide 1 Last modified by: user Created Date: 8/16/2006 12:00:00 AM Document presentation format: On-screen Show (4:3) Other titles: Arial Calibri Constantia ...
VOLONTERSTVO I CARITAS s. Jelena Lon ar, ravnateljica Caritasa Zagreba ke nadbiskupije 1. to je volonterstvo ili volontarijat ? ... (Caritas in veritate) ...
A. Sesana1, F. Haardt1, P. Madau2 The Final Parsec: Orbital Decay of Massive Black Holes in Galactic Stellar Cusps 1 Universita` dell'Insubria, via Valleggio 11 ...
Determining the dark energy equation of state from gravitational-wave (GW) observations of binary inspirals W.-T. Ni Department of Physics National Tsing Hua ...
MBHB M1 M2 on a Keplerian orbit with semimajor axis a and eccentricity e ... K is typically positive, but the eccentricity evoution of. the binary is modest ...
Mitch Begelman. JILA, University of Colorado. FORMATION AND ... YOU'VE GOT TO BE KIDDING. QUASISTAR PROPERTIES. Mass m* (M ) increases with time. Core with ...
* * * * * PSU group results (CV, Steffen, Just, Gibson)+Young+10 but see earlier Einstein results Lusso+10 for X-ray selected see poster by Antonucci Properties ...
Upravljanje financijama Napredna razina This project has been funded with support from the European Commission. This publication reflects the views only of the author ...
Quasars Quasi stellar radio sources, powerful, radio loud vs. ... Antonucci, R.: Unified models for active galactic nuclei and quasar, 1993, ARA&A, 31, 473A ...
Time it takes for black hole mass to increase by a factor of e if the quasar is shining at LEdd ... find that our black hole masses are consistent with those ...
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? ...
Galaxy formation starts with the invisid collapse of a uniform, constant omega rotating ... Thickness of galaxy, Sigma of galaxy at 10kpc = 0.035 g/cm2 ...
The VIRGO Cosmological N-body ... http://www.mpa-garching.mpg.de/galform/virgo ... Then, the likelihood that hmodel(t) is a good description of the data is ...
Thoeretical: Lars Hernquist (CfA), Volker Springel (MPA) ... SWIFT. GLAST. MAMBO. Exciting Era for High-z Objects. Presence of SMBH in quasars, MBH~109 M ...
Intermediate-Mass BHs and star clusters. Roberto Soria (CfA / University College London) ... old BHs, recycled systems? In globular. clusters? IMBH formation in ...
Martin Elvis, X-ray & XUV Active Optics, Soleil, 14-15 Dec 2006. Active X-ray Optics ... Martin Elvis. Harvard-Smithsonian Center for Astrophysics. Cambridge, ...
Dark Matter (DM) in haloes can dramatically alter the formation of the first ... I) Sufficiently High Dark Matter Density to get large annihilation rate ...
We conducted a visual inspection of 21,000 quasar spectra from the Sloan Digital ... This work is based on data from the Sloan Digital Sky Survey (http://www.sdss.org) ...
Cosmic stellar relics in the Galactic halo ... in Lya cooling halos (Tvir 104K ) ... The minimum and maximum (Mmin ,Mmax) halo mass in which star formation can ...