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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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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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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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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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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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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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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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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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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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Coevolution of black holes and galaxies at high redshift PowerPoint PPT Presentation
Coevolution of black holes and galaxies at high redshift - Coevolution of black holes and galaxies at high redshift David M Alexander (Durham)
Coevolution of black holes and galaxies at high redshift David M Alexander (Durham)
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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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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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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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Gravitational Waves from Massive BlackHole Binaries PowerPoint PPT Presentation
Gravitational Waves from Massive BlackHole Binaries - Gravitational Waves from Massive Black-Hole Binaries. Stuart Wyithe (U. Melb) NGC 6420 ... Regulation of growth during quasar phase. The quasar luminosity function. ...
Gravitational Waves from Massive Black-Hole Binaries. Stuart Wyithe (U. Melb) NGC 6420 ... Regulation of growth during quasar phase. The quasar luminosity function. ...
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Peeking into the Early Universe PowerPoint PPT Presentation
Peeking into the Early Universe - Peeking into the Early Universe
Peeking into the Early Universe
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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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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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2DRHD Simulations of superEddington BH accretion disks PowerPoint PPT Presentation
2DRHD Simulations of superEddington BH accretion disks - 2D-RHD Simulations of super-Eddington BH accretion disks. Ken OHSUGA (RIKEN, JAPAN) ... Accretion Disks. M- relation (see Silk & Rees 98; King 03) Conc. ...
2D-RHD Simulations of super-Eddington BH accretion disks. Ken OHSUGA (RIKEN, JAPAN) ... Accretion Disks. M- relation (see Silk & Rees 98; King 03) Conc. ...
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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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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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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 - Hard X-ray (10-600 keV) sky not yet surveyed to ROSAT sensitivity. ... Zenith pointer - scanning & nodding for full-sky coverage each orbit (95min) ...
Hard X-ray (10-600 keV) sky not yet surveyed to ROSAT sensitivity. ... Zenith pointer - scanning & nodding for full-sky coverage each orbit (95min) ...
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Diapositiva 1 PowerPoint PPT Presentation
Diapositiva 1 - 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 ...
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 ...
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Radio Loudness of AGNs: Host Galaxy Morphology and the Spin Paradigm PowerPoint PPT Presentation
Radio Loudness of AGNs: Host Galaxy Morphology and the Spin Paradigm - Radio Loudness of AGNs: Host Galaxy Morphology and the Spin Paradigm
Radio Loudness of AGNs: Host Galaxy Morphology and the Spin Paradigm
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Black holes: observations Lecture 5: Jets and lenses PowerPoint PPT Presentation
Black holes: observations Lecture 5: Jets and lenses - Black holes: observations Lecture 5: Jets and lenses Sergei Popov (SAI MSU) Plan and reviews Jets in AGNs and close binaries Close-by and far-away jets Classification ...
Black holes: observations Lecture 5: Jets and lenses Sergei Popov (SAI MSU) Plan and reviews Jets in AGNs and close binaries Close-by and far-away jets Classification ...
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Accretion to Neutron Stars and Black Holes in Binaries PowerPoint PPT Presentation
Accretion to Neutron Stars and Black Holes in Binaries - Distribution of ULXs in Galaxies ... in the halos of the galaxies. (Colbert & Ptak 2002) ... Detection of a strong narrow 54 mHz QPO in the starburst galaxy M82. ...
Distribution of ULXs in Galaxies ... in the halos of the galaxies. (Colbert & Ptak 2002) ... Detection of a strong narrow 54 mHz QPO in the starburst galaxy M82. ...
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Chandra Observations of Sgr A* PowerPoint PPT Presentation
Chandra Observations of Sgr A* - Title: Chandra Image of Sagittarius A* Field Author: Valued Sony Customer Last modified by: Valued Sony Customer Created Date: 1/3/2003 2:01:25 AM
Title: Chandra Image of Sagittarius A* Field Author: Valued Sony Customer Last modified by: Valued Sony Customer Created Date: 1/3/2003 2:01:25 AM
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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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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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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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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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The ubiquitous UV murmurs of sleeping supermassive BHs PowerPoint PPT Presentation
The ubiquitous UV murmurs of sleeping supermassive BHs - ... RARBRCRDRERFRGRHRIRJRKRLRMRNRORPRQRRRSRTRURVRWRXRYRZR[RR]R^R_R` ... 't' Jw 't' Jw 't' Jw 't' Jwb7GlE% Jw 't' Jw 't' Jw 't' Jw 't' Jw 't' Jw ...
... RARBRCRDRERFRGRHRIRJRKRLRMRNRORPRQRRRSRTRURVRWRXRYRZR[RR]R^R_R` ... 't' Jw 't' Jw 't' Jw 't' Jwb7GlE% Jw 't' Jw 't' Jw 't' Jw 't' Jw 't' Jw ...
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Binary Quasar Systems Gary Foreman PowerPoint PPT Presentation
Binary Quasar Systems Gary Foreman - 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 ...
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 ...
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Answers and questions from quasar surveys PowerPoint PPT Presentation
Answers and questions from quasar surveys - Answers (and questions) from quasar surveys. Scott Croom (IoA, University of Sydney) ... Stephen Fine (Sydney), Jose da Angela, Tom Shanks (Durham) ...
Answers (and questions) from quasar surveys. Scott Croom (IoA, University of Sydney) ... Stephen Fine (Sydney), Jose da Angela, Tom Shanks (Durham) ...
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Hard Xray Black Hole Surveys in Space and Time: EXIST Concept PowerPoint PPT Presentation
Hard Xray Black Hole Surveys in Space and Time: EXIST Concept - In 'Stanek Window' : probable. Wind-fed CVs, symbiotics (IPs?) (van den Berg et al 2006) ... CsI rear shields. Shields (GRB spectra to 10MeV) 0.72 m. 1.5 m ...
In 'Stanek Window' : probable. Wind-fed CVs, symbiotics (IPs?) (van den Berg et al 2006) ... CsI rear shields. Shields (GRB spectra to 10MeV) 0.72 m. 1.5 m ...
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Astrophysical Sources of Stochastic Gravitational-Wave Background PowerPoint PPT Presentation
Astrophysical Sources of Stochastic Gravitational-Wave Background - ... statistic (Drasco et al. 2003), Probability Event Horizon (Coward et al. 2005) ... Neutron star formation: Blair & Ju 1996, Coward et al. 2001-02, Howell et al. ...
... statistic (Drasco et al. 2003), Probability Event Horizon (Coward et al. 2005) ... Neutron star formation: Blair & Ju 1996, Coward et al. 2001-02, Howell et al. ...
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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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Black Holes and Revelations PowerPoint PPT Presentation
Black Holes and Revelations - * * * * * 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 ...
* * * * * 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 ...
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Conference Summary PowerPoint PPT Presentation
Conference Summary - These members have agreed to serve as the international advisory committee for ... Jets emanating from ergo sphere around a Kerr BH [S.Koide] ...
These members have agreed to serve as the international advisory committee for ... Jets emanating from ergo sphere around a Kerr BH [S.Koide] ...
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Dark Energy and the Hubble Constant PowerPoint PPT Presentation
Dark Energy and the Hubble Constant - What is dark energy (DE)? How does an accurate ( 3%) local measurement of the Hubble constant H0 plus ... Is DE a variable 'quintessence' ...
What is dark energy (DE)? How does an accurate ( 3%) local measurement of the Hubble constant H0 plus ... Is DE a variable 'quintessence' ...
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8.971: X-ray Astronomy PowerPoint PPT Presentation
8.971: X-ray Astronomy - 8.971: X-ray Astronomy Lecture 12 Super-Massive Black Holes, Jets, AGN, Quasars, Blazars Belinda Wilkes Chandra X-ray Center Smithsonian Astrophysical Observatory
8.971: X-ray Astronomy Lecture 12 Super-Massive Black Holes, Jets, AGN, Quasars, Blazars Belinda Wilkes Chandra X-ray Center Smithsonian Astrophysical Observatory
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IV : The effects of black holes on Galaxy formation PowerPoint PPT Presentation
IV : The effects of black holes on Galaxy formation - The Hot Big Bang. Dark Matter Dynamics. The main steps of galaxy formation ... Velocity dispersion is most directly related to the mass of the galactic bulge ...
The Hot Big Bang. Dark Matter Dynamics. The main steps of galaxy formation ... Velocity dispersion is most directly related to the mass of the galactic bulge ...
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The%20other%20side%20of%20galaxy%20formation:%20radio%20deep%20fields PowerPoint PPT Presentation
The%20other%20side%20of%20galaxy%20formation:%20radio%20deep%20fields - The other side of galaxy formation: radio deep fields
The other side of galaxy formation: radio deep fields
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Blazar Variability PowerPoint PPT Presentation
Blazar Variability - Blazar Variability
Blazar Variability
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Diapositive 1 PowerPoint PPT Presentation
Diapositive 1 - G nter Sigl, Astroparticules et Cosmologie, Paris. Data analysis workshop, Paris, ... G nter Sigl. APC (Astroparticule et Cosmologie), Universit Paris 7 ...
G nter Sigl, Astroparticules et Cosmologie, Paris. Data analysis workshop, Paris, ... G nter Sigl. APC (Astroparticule et Cosmologie), Universit Paris 7 ...
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Supermassive Black Holes PowerPoint PPT Presentation
Supermassive Black Holes - Supermassive Black Holes
Supermassive Black Holes
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Star Formation at Very Low Metallicities PowerPoint PPT Presentation
Star Formation at Very Low Metallicities - Star Formation at Very Low Metallicities
Star Formation at Very Low Metallicities
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Dark Matter Halo Mergers PowerPoint PPT Presentation
Dark Matter Halo Mergers - Dark Matter Halo Mergers
Dark Matter Halo Mergers
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ESO PowerPoint PPT Presentation
ESO - The other side of galaxy formation: radio line and continuum ... Extreme gas rich galaxies without extreme starbursts. Gas depletion timescales 5 x108 yrs ...
The other side of galaxy formation: radio line and continuum ... Extreme gas rich galaxies without extreme starbursts. Gas depletion timescales 5 x108 yrs ...
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Marta Volonteri PowerPoint PPT Presentation
Marta Volonteri - BULGE. tiny BHs know about big bulges! MBHs 106-109 Msun. What is a galaxy made of? ... The universe after the Big Bang was not completely uniform ...
BULGE. tiny BHs know about big bulges! MBHs 106-109 Msun. What is a galaxy made of? ... The universe after the Big Bang was not completely uniform ...
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P1253553533cBXEt PowerPoint PPT Presentation
P1253553533cBXEt - ... Energy Density. Gas ... Density & Velocity fields. Outflow. Bubbles & Circular ... Radiation Energy Density. Radiation Pressure. Gas Pressure. Gas ...
... Energy Density. Gas ... Density & Velocity fields. Outflow. Bubbles & Circular ... Radiation Energy Density. Radiation Pressure. Gas Pressure. Gas ...
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Some Astrophysical Implications from Dark Matter Neutralino Annihilation PowerPoint PPT Presentation
Some Astrophysical Implications from Dark Matter Neutralino Annihilation - Very close to the EGRET upper limit for a cluster @ 100Mpc. Many positional coincidence between clusters and un-ID EGRET sources (e.g. Reimer et al. 2003) ...
Very close to the EGRET upper limit for a cluster @ 100Mpc. Many positional coincidence between clusters and un-ID EGRET sources (e.g. Reimer et al. 2003) ...
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Introduction to Gravitational Waves PowerPoint PPT Presentation
Introduction to Gravitational Waves - Need 100kW of laser power in arms, use power recycling so that laser ... Crab Spindown. Upper Limit. Known Pulsars: First Interferometers: 3x10-6 (1000Hz/f) ...
Need 100kW of laser power in arms, use power recycling so that laser ... Crab Spindown. Upper Limit. Known Pulsars: First Interferometers: 3x10-6 (1000Hz/f) ...
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BLACK HOLES: FROM STARS TO GALAXIES PowerPoint PPT Presentation
BLACK HOLES: FROM STARS TO GALAXIES - for the existence of BHs as stellar remnants in binaries, ... Inflow of mass & jet collimation close to the BH in terms of the gravitational ...
for the existence of BHs as stellar remnants in binaries, ... Inflow of mass & jet collimation close to the BH in terms of the gravitational ...
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