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The Coevolution of SMBHs PowerPoint PPT Presentation
The Coevolution of SMBHs - The Coevolution of SMBHs
The Coevolution of SMBHs
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Joint formation and evolution of SMBHs and their host galaxies: PowerPoint PPT Presentation
Joint formation and evolution of SMBHs and their host galaxies: - 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
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
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Growth of SMBH: the connection between accretion physics and Cosmology PowerPoint PPT Presentation
Growth of SMBH: the connection between accretion physics and Cosmology - the connection between accretion physics and Cosmology. PASBH Santa Fe 11/07/2006 ... Constraints on accretion efficiency via Soltan-type arguments ...
the connection between accretion physics and Cosmology. PASBH Santa Fe 11/07/2006 ... Constraints on accretion efficiency via Soltan-type arguments ...
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Growth of SMBH studied through X-ray surveys PowerPoint PPT Presentation
Growth of SMBH studied through X-ray surveys - 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) ...
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) ...
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Modeling the Accretion Flow Around the SMBH at the Galactic Center PowerPoint PPT Presentation
Modeling the Accretion Flow Around the SMBH at the Galactic Center - Muduleya LEI HUANG @SINO-GERMAN. 1 ... Center for Astrophysics, USTC. Collaborators: Zhi-Qiang Shen, ... Magneto-Rotational-Instability (MRI) Mechanism ...
Muduleya LEI HUANG @SINO-GERMAN. 1 ... Center for Astrophysics, USTC. Collaborators: Zhi-Qiang Shen, ... Magneto-Rotational-Instability (MRI) Mechanism ...
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Measuring SMBH parameters with LISA PowerPoint PPT Presentation
Measuring SMBH parameters with LISA - Brans-Dicke: dipole radiation - best bounds from NS-IMBH systems ... Needed astrophysical input for optimal data analysis before LISA flies: ...
Brans-Dicke: dipole radiation - best bounds from NS-IMBH systems ... Needed astrophysical input for optimal data analysis before LISA flies: ...
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The build-up of SMBHs in z<1 red galaxies PowerPoint PPT Presentation
The build-up of SMBHs in z<1 red galaxies - ... 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 ...
... 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 ...
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ALMA: Imaging the cold Universe PowerPoint PPT Presentation
ALMA: Imaging the cold Universe - Coeval formation of SMBH/Galaxy? Dust formation by massive stars? ... coeval formation of SMBH/Galaxy? Break-down of M- relation at high z? ...
Coeval formation of SMBH/Galaxy? Dust formation by massive stars? ... coeval formation of SMBH/Galaxy? Break-down of M- relation at high z? ...
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The Transient Radio Sky Astrophysical and Artificial PowerPoint PPT Presentation
The Transient Radio Sky Astrophysical and Artificial - ... disk surrounding a SMBH = coeval SMBH galaxy formation? ... M-s relation coeval SMBH and galaxy formation? QSO dust heating: star formation or AGN? ...
... 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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Les examens biologiques en H PowerPoint PPT Presentation
Les examens biologiques en H - 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 ...
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 ...
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Accretion%20vs%20Star%20Formation PowerPoint PPT Presentation
Accretion%20vs%20Star%20Formation - Accretion onto the SMBH releases electromagnetic radiations creates quasars and AGN ... undergoing inefficient accretion ... out of plane of accretion disk ...
Accretion onto the SMBH releases electromagnetic radiations creates quasars and AGN ... undergoing inefficient accretion ... out of plane of accretion disk ...
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Obscured AGN in the (z)COSMOS survey PowerPoint PPT Presentation
Obscured AGN in the (z)COSMOS survey - ... COSMOS survey Complete census of ... Hierarchical growth Growth of SMBH Gas inflow AGN feedback Active Quasar Starburst & buried Quasar Normal galaxies Galaxy ...
... COSMOS survey Complete census of ... Hierarchical growth Growth of SMBH Gas inflow AGN feedback Active Quasar Starburst & buried Quasar Normal galaxies Galaxy ...
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Supermassive binary black holes in powerful AGN PowerPoint PPT Presentation
Supermassive binary black holes in powerful AGN - Supermassive binary black holes in powerful AGN. Andrei Lobanov ... Questions of relativistic jets and binary SMBH. Relativistic jets from binary SMBH: the case ...
Supermassive binary black holes in powerful AGN. Andrei Lobanov ... Questions of relativistic jets and binary SMBH. Relativistic jets from binary SMBH: the case ...
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Roberto Soria (CfA) PowerPoint PPT Presentation
Roberto Soria (CfA) - 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? ...
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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Science Synergies with NRAO Telescopes PowerPoint PPT Presentation
Science Synergies with NRAO Telescopes - 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 ...
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 ...
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Black Hole Masses and Accretion Rates Through the AGES PowerPoint PPT Presentation
Black Hole Masses and Accretion Rates Through the AGES - Why care about Supermassive Black Hole (SMBH) masses and feeding rates? ... From Steed & Weinberg 2003. Want to Probe the 'knee' a1. a2 ...
Why care about Supermassive Black Hole (SMBH) masses and feeding rates? ... From Steed & Weinberg 2003. Want to Probe the 'knee' a1. a2 ...
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The BlackHole Halo Mass Relation and High Redshift Quasars PowerPoint PPT Presentation
The BlackHole Halo Mass Relation and High Redshift Quasars - The bulges of all local galaxies contain SMBHs. ... At higher redshift, galaxies form out of a denser background, have a larger ...
The bulges of all local galaxies contain SMBHs. ... At higher redshift, galaxies form out of a denser background, have a larger ...
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Deep Extragalactic Xray Surveys W.N. Brandt PSU, G. Hasinger MPE, 2005, ARAA, 43, 827 astroph0501058 PowerPoint PPT Presentation
Deep Extragalactic Xray Surveys W.N. Brandt PSU, G. Hasinger MPE, 2005, ARAA, 43, 827 astroph0501058 - X-ray Measurements of AGN Evolution and the Growth of SMBH ... the 1970's revealed a high degree of CXRB isotropy CXRB mainly extragalactic. ...
X-ray Measurements of AGN Evolution and the Growth of SMBH ... the 1970's revealed a high degree of CXRB isotropy CXRB mainly extragalactic. ...
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The Next Nearest BH Open Univ Dec 2004 PowerPoint PPT Presentation
The Next Nearest BH Open Univ Dec 2004 - M31* - The Nearest Extra-Galactic SMBH. Michael Garcia, Smithsonian ... Position of Crane 1992 pt radio source? ( within 0.5'', accurate to 0.15''...) ~1' ...
M31* - The Nearest Extra-Galactic SMBH. Michael Garcia, Smithsonian ... Position of Crane 1992 pt radio source? ( within 0.5'', accurate to 0.15''...) ~1' ...
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Promotion de la sant PowerPoint PPT Presentation
Promotion de la sant - 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 ...
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 ...
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Galaxies and Quasars in the Epoch of Reionization PowerPoint PPT Presentation
Galaxies and Quasars in the Epoch of Reionization - Thoeretical: Lars Hernquist (CfA), Volker Springel (MPA) ... SWIFT. GLAST. MAMBO. Exciting Era for High-z Objects. Presence of SMBH in quasars, MBH~109 M ...
Thoeretical: Lars Hernquist (CfA), Volker Springel (MPA) ... SWIFT. GLAST. MAMBO. Exciting Era for High-z Objects. Presence of SMBH in quasars, MBH~109 M ...
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The Chandra survey of the COSMOS field PowerPoint PPT Presentation
The Chandra survey of the COSMOS field - ... in the most local bulges; tight correlation between MBH and bulge properties. ... Most bulges passed a phase of activity: Complete SMBH census, ...
... in the most local bulges; tight correlation between MBH and bulge properties. ... Most bulges passed a phase of activity: Complete SMBH census, ...
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ALMA Presentation PowerPoint PPT Presentation
ALMA Presentation - Epoch of Reionization. last phase of cosmic evolution to be explored ... Coeval formation of SMBH ... Coeval formation SMBH Host Gal. Break-down MBH-Mbulge ...
Epoch of Reionization. last phase of cosmic evolution to be explored ... Coeval formation of SMBH ... Coeval formation SMBH Host Gal. Break-down MBH-Mbulge ...
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Mutual feedback between star formation and nuclear activity at high z Implications for Galaxy Formation Models PowerPoint PPT Presentation
Mutual feedback between star formation and nuclear activity at high z Implications for Galaxy Formation Models - Mutual feedback between star formation and nuclear activity at high z Implications for Galaxy Formation Models Gian Luigi Granato INAF and SISSA
Mutual feedback between star formation and nuclear activity at high z Implications for Galaxy Formation Models Gian Luigi Granato INAF and SISSA
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Supermassive Black Hole Growth from Cosmological N-body Simulations PowerPoint PPT Presentation
Supermassive Black Hole Growth from Cosmological N-body Simulations - a few isolated halos have extremely underweight bhs Following the leads with better dynamics gravitational wave kicks!
a few isolated halos have extremely underweight bhs Following the leads with better dynamics gravitational wave kicks!
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Supermassive black holes PowerPoint PPT Presentation
Supermassive black holes - ... 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 ...
... 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 ...
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AMUSE-Virgo AGN Multi-wavelength Survey in Early type galaxies PowerPoint PPT Presentation
AMUSE-Virgo AGN Multi-wavelength Survey in Early type galaxies - AMUSE: science goals ... AMUSE: the survey ... AMUSE: first Chandra results II. ...
AMUSE: science goals ... AMUSE: the survey ... AMUSE: first Chandra results II. ...
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Aucun titre de diapositive PowerPoint PPT Presentation
Aucun titre de diapositive - Les Etudes Scientifiques l Universit et le syst me LMD Mission acad mique pour les Sciences Universit s Paris 8, Paris 12, Paris 13 et Marne la Vall e
Les Etudes Scientifiques l Universit et le syst me LMD Mission acad mique pour les Sciences Universit s Paris 8, Paris 12, Paris 13 et Marne la Vall e
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Supermassive Black Hole Binaries in AGNs PowerPoint PPT Presentation
Supermassive Black Hole Binaries in AGNs - Laser Interferometer Space Antenna (LISA) (Danzmann 2003) ... LISA: 10-4-10-1 Hz (MBH 104 -107M) ESA & NASA: Laser Interferometer Space Antenna (LISA) in 2018 ...
Laser Interferometer Space Antenna (LISA) (Danzmann 2003) ... LISA: 10-4-10-1 Hz (MBH 104 -107M) ESA & NASA: Laser Interferometer Space Antenna (LISA) in 2018 ...
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eLISA (or NGO): the New LISA PowerPoint PPT Presentation
eLISA (or NGO): the New LISA - eLISA (or NGO): the New LISA Gijs Nelemans Radboud University Nijmegen Some history on GW detector in space Low-frequency gravitational wave mission first proposed in ...
eLISA (or NGO): the New LISA Gijs Nelemans Radboud University Nijmegen Some history on GW detector in space Low-frequency gravitational wave mission first proposed in ...
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Tut PowerPoint PPT Presentation
Tut - Tut Rentr e Ou comment bien commencer son ann e Qui me parle ? Stephanie DA SILVA, VP tutorat. Contact: tutorat.p13@hotmail.fr BIENVENUE BOBIGNY La FAC: ...
Tut Rentr e Ou comment bien commencer son ann e Qui me parle ? Stephanie DA SILVA, VP tutorat. Contact: tutorat.p13@hotmail.fr BIENVENUE BOBIGNY La FAC: ...
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H2O Masers and AGN Structure PowerPoint PPT Presentation
H2O Masers and AGN Structure - Consider the Circinus galaxy... Jones et al. (1999) Veilleux ... In Circinus, conditions. support H2O masers in. an edge-on accretion disk. a nuclear outflow ...
Consider the Circinus galaxy... Jones et al. (1999) Veilleux ... In Circinus, conditions. support H2O masers in. an edge-on accretion disk. a nuclear outflow ...
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Formation and Evolution of Supermassive binary black holes in AGNs PowerPoint PPT Presentation
Formation and Evolution of Supermassive binary black holes in AGNs - Title: Formation and Evolution of Supermassive binary black holes in AGNs Author: Fukun Liu Last modified by: liu Created Date: 12/23/2003 1:03:12 PM
Title: Formation and Evolution of Supermassive binary black holes in AGNs Author: Fukun Liu Last modified by: liu Created Date: 12/23/2003 1:03:12 PM
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SuperMassive Black Holes: PowerPoint PPT Presentation
SuperMassive Black Holes: - Title: Presentazione di PowerPoint Author: Pasotti Francesco Last modified by: Guido Chincarini Created Date: 6/27/2005 6:29:45 PM Document presentation format
Title: Presentazione di PowerPoint Author: Pasotti Francesco Last modified by: Guido Chincarini Created Date: 6/27/2005 6:29:45 PM Document presentation format
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Active Galactic Nuclei PowerPoint PPT Presentation
Active Galactic Nuclei - The profile is skewed with an extended red wing due to gravitational redshift, ... Sagittarius A* An unresolved bright continuum at radio wavelengths ...
The profile is skewed with an extended red wing due to gravitational redshift, ... Sagittarius A* An unresolved bright continuum at radio wavelengths ...
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ACTIVE%20GALACTIC%20NUCLEI%20and%20UNIFICATION%20SCHEMES PowerPoint PPT Presentation
ACTIVE%20GALACTIC%20NUCLEI%20and%20UNIFICATION%20SCHEMES - ACTIVE GALACTIC NUCLEI and UNIFICATION SCHEMES
ACTIVE GALACTIC NUCLEI and UNIFICATION SCHEMES
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Realistic Rates for the Detection of Supermassive Black Hole coalescence by LISA PowerPoint PPT Presentation
Realistic Rates for the Detection of Supermassive Black Hole coalescence by LISA - Realistic Rates for the Detection of Supermassive Black Hole coalescence by LISA ... Ringdown phase: quadrupole distortion to rotating (Kerr) black hole ...
Realistic Rates for the Detection of Supermassive Black Hole coalescence by LISA ... Ringdown phase: quadrupole distortion to rotating (Kerr) black hole ...
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Black hole formation PowerPoint PPT Presentation
Black hole formation - Black hole formation ( ) 1. Astrophysical black holes 2. Formation of black holes 3. Evolution of black holes Ref: Proc. Carnegie sympo ...
Black hole formation ( ) 1. Astrophysical black holes 2. Formation of black holes 3. Evolution of black holes Ref: Proc. Carnegie sympo ...
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Sgr A* PowerPoint PPT Presentation
Sgr A* - Sgr A
Sgr A
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AGN Demographics PowerPoint PPT Presentation
AGN Demographics - ... Ratio is independent of stellar mass AGN not related to quenching or color change Aird 12 More in Blue/Green by factor of 2 z ~ 1 ... is a Demographical ...
... Ratio is independent of stellar mass AGN not related to quenching or color change Aird 12 More in Blue/Green by factor of 2 z ~ 1 ... is a Demographical ...
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To measure the brightness distribution of galaxies, we must determine the surface brightness of the resolved galaxy. PowerPoint PPT Presentation
To measure the brightness distribution of galaxies, we must determine the surface brightness of the resolved galaxy. - Photometric Properties of Galaxies To measure the brightness distribution of galaxies, we must determine the surface brightness of the resolved galaxy.
Photometric Properties of Galaxies To measure the brightness distribution of galaxies, we must determine the surface brightness of the resolved galaxy.
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Diapositive 1 PowerPoint PPT Presentation
Diapositive 1 - Astrophysical Gravitational Wave Backgrounds Cosmological supernovae as neutrino and gravitational wave sources mHz gravitational wave background from inspiral of ...
Astrophysical Gravitational Wave Backgrounds Cosmological supernovae as neutrino and gravitational wave sources mHz gravitational wave background from inspiral of ...
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Astrometry William F. van Altena ARAA (1983) PowerPoint PPT Presentation
Astrometry William F. van Altena ARAA (1983) - Title: Recent Advances in Astrometry with the VLBA Author: mark reid Last modified by: mark reid Created Date: 2/10/2005 1:54:39 PM Document presentation format
Title: Recent Advances in Astrometry with the VLBA Author: mark reid Last modified by: mark reid Created Date: 2/10/2005 1:54:39 PM Document presentation format
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Galaxies actives PowerPoint PPT Presentation
Galaxies actives - Galaxies actives Vue d ensemble Trous noirs et accr tion Composants de l AGN Unification Quasars et cosmologie ...
Galaxies actives Vue d ensemble Trous noirs et accr tion Composants de l AGN Unification Quasars et cosmologie ...
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Galaxy Evolution and WFMOS PowerPoint PPT Presentation
Galaxy Evolution and WFMOS - Galaxy Evolution and WFMOS History of Galaxies Present-day Universe: SDSS WFMOS Survey of z1 Universe K. Shimasaku (University of Tokyo) galaxy morphology galaxy ...
Galaxy Evolution and WFMOS History of Galaxies Present-day Universe: SDSS WFMOS Survey of z1 Universe K. Shimasaku (University of Tokyo) galaxy morphology galaxy ...
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Massive galaxy (and black hole) formation in the early Universe PowerPoint PPT Presentation
Massive galaxy (and black hole) formation in the early Universe - Fine structure lines: dominant ISM gas coolant ... Index = 1. FIR -- HCN = linear relation from GMCs to HyLIRGs ... Rapid enrichment of metals, dust in ISM (z 8) ...
Fine structure lines: dominant ISM gas coolant ... Index = 1. FIR -- HCN = linear relation from GMCs to HyLIRGs ... Rapid enrichment of metals, dust in ISM (z 8) ...
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Radio astronomical probes of Cosmic Reionization and the 1st luminous objects PowerPoint PPT Presentation
Radio astronomical probes of Cosmic Reionization and the 1st luminous objects - Radio astronomical probes of Cosmic Reionization and the 1st luminous objects
Radio astronomical probes of Cosmic Reionization and the 1st luminous objects
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Radio astronomical probes of cosmic reionization and the first galaxies PowerPoint PPT Presentation
Radio astronomical probes of cosmic reionization and the first galaxies - Radio astronomical probes of cosmic reionization and the first galaxies
Radio astronomical probes of cosmic reionization and the first galaxies
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Diapositiva 1 PowerPoint PPT Presentation
Diapositiva 1 - 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 ...
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 ...
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EXIST Concept for BHFP: Hard X-ray Black Hole Surveys in Space and Time PowerPoint PPT Presentation
EXIST Concept for BHFP: Hard X-ray Black Hole Surveys in Space and Time - Title: PowerPoint Presentation Last modified by: Sandy Grindlay Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles
Title: PowerPoint Presentation Last modified by: Sandy Grindlay Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles
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High-z (z > 3) QSOs studied with Subaru/HSC PowerPoint PPT Presentation
High-z (z > 3) QSOs studied with Subaru/HSC - Richards et al. (2001) g' r' r' i' r' i' i' z'. Selection in ... Richards et al. (2006) Schneider et al. (2005) 46420 QSOs. in SDSS DR3. 0 1 2 3 4 5 ...
Richards et al. (2001) g' r' r' i' r' i' i' z'. Selection in ... Richards et al. (2006) Schneider et al. (2005) 46420 QSOs. in SDSS DR3. 0 1 2 3 4 5 ...
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Radio observations of massive galaxy and black hole formation in the early Universe PowerPoint PPT Presentation
Radio observations of massive galaxy and black hole formation in the early Universe - Radio observations of massive galaxy and black hole formation in the early Universe
Radio observations of massive galaxy and black hole formation in the early Universe
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The nuclear activity of late-type galaxies in the Virgo Cluster PowerPoint PPT Presentation
The nuclear activity of late-type galaxies in the Virgo Cluster - Universit degli Studi di Milano Bicocca Dipartimento di Fisica Universit degli Studi dell Insubria Dipartimento di Fisica e Matematica
Universit degli Studi di Milano Bicocca Dipartimento di Fisica Universit degli Studi dell Insubria Dipartimento di Fisica e Matematica
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Blank PowerPoint PPT Presentation
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Paul O PowerPoint PPT Presentation
Paul O - Carl Seyfert (1943) Postdoc at Mount Wilson ... Magdalena Ridge Observatory, NM 10 x 1.4m optical/IR telescopes with baselines ...
Carl Seyfert (1943) Postdoc at Mount Wilson ... Magdalena Ridge Observatory, NM 10 x 1.4m optical/IR telescopes with baselines ...
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ALMA%20Presentation PowerPoint PPT Presentation
ALMA%20Presentation - Not event', but complex process, large variance time/space ... High order, fine structure lines. Detect dust emission in 1sec (5 ) at 250 GHz ...
Not event', but complex process, large variance time/space ... High order, fine structure lines. Detect dust emission in 1sec (5 ) at 250 GHz ...
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