... UK), J. Binney (Oxford, UK), T. Statler (Ohio, USA), T. de Zeeuw (Leiden, NL) ... (SMBHs) are the only viable candidates for the massive dark objects inferred ...
Title: The BH mass of nearby QSOs Author: Marzia Last modified by: Marzia Created Date: 3/27/2006 1:09:12 PM Document presentation format: Presentazione su schermo
HST Workshop Bologna Jan 31, 2008. Heavily obscured SMBH at high redshift. Andrea ... HST Workshop Bologna Jan 31, 2008. 135 sources (out of 1729 with F24 40 ...
Title: PowerPoint Presentation Last modified by: Elena Created Date: 1/1/1601 12:00:00 AM Document presentation format: Presentazione su schermo Other titles
Chandra and Spitzer imaging. Stacking the X-ray images gives a highly significant signal ... X-ray images in different subsets of the data to obtain a mean ...
Local galaxies all harbor SMBH (from stellar and gas ... Big blue bump a =2 (Rayleigh Jeans tail) Power law reflection component in the X-ray ( 1 keV) ...
the connection between accretion physics and Cosmology. PASBH Santa Fe 11/07/2006 ... Constraints on accretion efficiency via Soltan-type arguments ...
... XBootes survey to stack up the X-ray images to obtain a mean X-ray luminosity. ... Although X-ray emission is likely to be dominated by AGN activity, infrared ...
Les examens biologiques en H matologie R mi Letestu Laboratoire d H matologie CHU Avicenne UFR SMBH DCEM1 (2006-07) H matopo se Les diff rents examens Les ...
Supermassive Black Hole Growth and Merger ... to have gas accreting SMBH, it is easy to grow Sagittarius A* size black hole. ... Sagittarius A* M31 SMBH. 14 ...
Quasars and Galaxy Formation. By Joseph Silk and Martin J. Rees. 1997 ... High Star formation rates near SMBH. Star Formation stimulated by SMBH. Conclusions ...
Supermassive binary black holes in powerful AGN. Andrei Lobanov ... Questions of relativistic jets and binary SMBH. Relativistic jets from binary SMBH: the case ...
[D = 1 Gpc; eccentric orbit and non-spinning SMBH] (Barack and ... For binary systems at D ~ 1 Gpc: IMBH and SMBH mass with fractional error 1 part in 10,000 ...
Accretion onto the SMBH releases electromagnetic radiations creates quasars and AGN ... undergoing inefficient accretion ... out of plane of accretion disk ...
... COSMOS survey Complete census of ... Hierarchical growth Growth of SMBH Gas inflow AGN feedback Active Quasar Starburst & buried Quasar Normal galaxies Galaxy ...
Some Possible Sources of Burst Radiation. Formation of SMBH (Thorne and Braginski 76) ... Sensitivity to a 0.75 s 2-week burst, daily observing, 20 pulsars ...
LISA (Laser Interferometer Space Antenna) LIASE (Laser Interferometer Arc-Second Explorer) ... LISA Science. Detect every SMBH & IMBH binary merger in the Universe ...
M31* - The Nearest Extra-Galactic SMBH. Michael Garcia, Smithsonian ... Position of Crane 1992 pt radio source? ( within 0.5'', accurate to 0.15''...) ~1' ...
Epoch of Reionization. last phase of cosmic evolution to be explored ... Coeval formation of SMBH ... Coeval formation SMBH Host Gal. Break-down MBH-Mbulge ...
z 6 = Low order molecular transitions redshift to the short ... coeval formation of giant elliptical galaxy SMBH within 870 Myr of Big Bang. 1' CII CO 3-2 ...
Galactic Astronomy. Precession of the SMBH in NGC 1275? Dong-hyun Lee. 2007/05/28. Radio bubbles of the Perseus cluster. Radio bubbles of the Perseus cluster ...
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? ...
Obscured (hard) X ray emission SMBH is present and the host galaxy is visible ... X-ray-to-optical color (X/O 10) photometric redshift (zphot 1) (adapted from ...
Promotion de la sant et Pr vention Rep res conceptuels et strat gies d action face aux In galit s Sociales de Sant Pierre LOMBRAIL, PU (SMBH, Paris 13 ...
Thoeretical: Lars Hernquist (CfA), Volker Springel (MPA) ... SWIFT. GLAST. MAMBO. Exciting Era for High-z Objects. Presence of SMBH in quasars, MBH~109 M ...
... in the most local bulges; tight correlation between MBH and bulge properties. ... Most bulges passed a phase of activity: Complete SMBH census, ...
GEZARI ET AL. 2007. UV/Optical Detections of Candidate ... How are SMBH masses derived? OIII kinematics M-s* Relations with bulge mass / luminosity M-L ...
Title: Blacks Holes Lecture 6 Slideshow Author: N. Brandt, for PSIWA Last modified by: William Brandt Created Date: 7/3/2008 3:44:11 PM Document presentation format
But if BH in binary, pericenter distance can be much greater, hence cross section higher. ... Key: calculation of binary fraction and properties. Single-body ...
Realistic Rates for the Detection of Supermassive Black Hole coalescence by LISA ... Ringdown phase: quadrupole distortion to rotating (Kerr) black hole ...
Distance to the Galactic center: 26,000 light-year. ... Detailed structure of ionized gas pillars sculpted by the intense radiation and wind from the Quintuplet ...
Title: Presentazione di PowerPoint Author: Pasotti Francesco Last modified by: Guido Chincarini Created Date: 6/27/2005 6:29:45 PM Document presentation format
Linqing Wen. AEI. Germany. Teviet Creighton. Caltech. USA. John Armstrong. JPL. USA. What can we do with an array of pulsars and the G-wave background? ...
... of Sgr A* Constraints on the size of Sgr A* M31 A large BH in M31 Active galactic nuclei and quasars Quasars spectra ... BH interpretation ... UV) . flat ...
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 ...
Laura Silva ... Since long (Silva et al 1998, Granato et al 2001, 2004) we have devoted efforts ... Silva et al 2005. Star forming. Passive. Adapted from Drory ...
University of Texas at Brownsville. Collaborators. Dick Manchester. ATNF/CSIRO. Australia ... Teviet Creighton. Caltech. USA. John Armstrong. JPL. USA. Main Points ...