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Largest SMBH PowerPoint PPT Presentation
Largest SMBH - ... 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 ...
... 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 ...
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The cosmic spin of SMBHs from radio observations PowerPoint PPT Presentation
The cosmic spin of SMBHs from radio observations - Leiden, Feb 2011 Assumptions: Accretion rate Jet power Bolometric Luminosity e.g. Mckinney (2005), Hawley & Krolik (2006), Nemmen et al. (2007), Benson & Babul ...
Leiden, Feb 2011 Assumptions: Accretion rate Jet power Bolometric Luminosity e.g. Mckinney (2005), Hawley & Krolik (2006), Nemmen et al. (2007), Benson & Babul ...
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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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Heavily obscured SMBH at high redshift PowerPoint PPT Presentation
Heavily obscured SMBH at high redshift - 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 ...
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 ...
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On the inconsistency between the SMBH Mass Function from velocity dispersion and luminosity PowerPoint PPT Presentation
On the inconsistency between the SMBH Mass Function from velocity dispersion and luminosity - Title: PowerPoint Presentation Last modified by: Elena Created Date: 1/1/1601 12:00:00 AM Document presentation format: Presentazione su schermo Other titles
Title: PowerPoint Presentation Last modified by: Elena Created Date: 1/1/1601 12:00:00 AM Document presentation format: Presentazione su schermo Other titles
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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 Accretion History of SMBHs in Massive Galaxies PowerPoint PPT Presentation
The Accretion History of SMBHs in Massive Galaxies - 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 ...
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 ...
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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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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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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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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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Cosmological Evolution of Hard Xray AGN Luminosity Function: Formation History of the SMBHs PowerPoint PPT Presentation
Cosmological Evolution of Hard Xray AGN Luminosity Function: Formation History of the SMBHs - Fabian and Iwasawa (1999) , Elvis et al (2002) ... is marginally consistent with the present-day BH mass density from the SDSS, ...
Fabian and Iwasawa (1999) , Elvis et al (2002) ... is marginally consistent with the present-day BH mass density from the SDSS, ...
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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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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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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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Supermassive Black Hole Growth and Merger Rates From Cosmological N-Body Simulations PowerPoint PPT Presentation
Supermassive Black Hole Growth and Merger Rates From Cosmological N-Body Simulations - 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 ...
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 ...
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L PowerPoint PPT Presentation
L - Title: Environnement naturel = Espace habituel Author: UFR SMBH - ARPE Last modified by: Sophie Bomo Created Date: 11/10/2000 12:19:48 PM Document presentation format
Title: Environnement naturel = Espace habituel Author: UFR SMBH - ARPE Last modified by: Sophie Bomo Created Date: 11/10/2000 12:19:48 PM Document presentation format
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Quasars and Galaxy Formation PowerPoint PPT Presentation
Quasars and Galaxy Formation - Quasars and Galaxy Formation. By Joseph Silk and Martin J. Rees. 1997 ... High Star formation rates near SMBH. Star Formation stimulated by SMBH. Conclusions ...
Quasars and Galaxy Formation. By Joseph Silk and Martin J. Rees. 1997 ... High Star formation rates near SMBH. Star Formation stimulated by SMBH. Conclusions ...
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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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Astrophysics to be learned from observations of intermediate mass black hole inspiral events PowerPoint PPT Presentation
Astrophysics to be learned from observations of intermediate mass black hole inspiral events - [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 ...
[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 ...
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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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Pulsar Array Gravitational-wave Observatory PowerPoint PPT Presentation
Pulsar Array Gravitational-wave Observatory - 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 ...
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 ...
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LISA and Beyond PowerPoint PPT Presentation
LISA and Beyond - LISA (Laser Interferometer Space Antenna) LIASE (Laser Interferometer Arc-Second Explorer) ... LISA Science. Detect every SMBH & IMBH binary merger in the Universe ...
LISA (Laser Interferometer Space Antenna) LIASE (Laser Interferometer Arc-Second Explorer) ... LISA Science. Detect every SMBH & IMBH binary merger in the Universe ...
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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 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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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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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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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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Galactic Astronomy PowerPoint PPT Presentation
Galactic Astronomy - 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 ...
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 ...
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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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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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Obscured AGN in the COSMOS field PowerPoint PPT Presentation
Obscured AGN in the COSMOS field - 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 ...
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 ...
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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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Gezari et al' 2007 PowerPoint PPT Presentation
Gezari et al' 2007 - 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 ...
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 ...
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Lecture 14: Supermassive Black Holes in Hibernation PowerPoint PPT Presentation
Lecture 14: Supermassive Black Holes in Hibernation - 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
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
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Magorrian relation 2nd stage ? PowerPoint PPT Presentation
Magorrian relation 2nd stage ? - Magorrian relation 2nd stage BH MDO (Massive Dark Object) BH-bulge MDO-bulge BH ...
Magorrian relation 2nd stage BH MDO (Massive Dark Object) BH-bulge MDO-bulge BH ...
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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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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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Gravitational Wave Sources From Dense Star Clusters PowerPoint PPT Presentation
Gravitational Wave Sources From Dense Star Clusters - But if BH in binary, pericenter distance can be much greater, hence cross section higher. ... Key: calculation of binary fraction and properties. Single-body ...
But if BH in binary, pericenter distance can be much greater, hence cross section higher. ... Key: calculation of binary fraction and properties. Single-body ...
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Pr PowerPoint PPT Presentation
Pr - SUZY COLLIN-ZAHN Lodewick Woltjer lecture EWASS, Turku, July 11, 2013
SUZY COLLIN-ZAHN Lodewick Woltjer lecture EWASS, Turku, July 11, 2013
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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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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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A Panoramic HST Infrared View of the Galactic Center PowerPoint PPT Presentation
A Panoramic HST Infrared View of the Galactic Center - 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 ...
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 ...
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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: - 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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Detecting the Gravitational Wave background using Millisecond Pulsars PowerPoint PPT Presentation
Detecting the Gravitational Wave background using Millisecond Pulsars - 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? ...
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? ...
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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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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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The joint formation of spheroids and Super Massive Black Holes Gian Luigi Granato INAFPadova PowerPoint PPT Presentation
The joint formation of spheroids and Super Massive Black Holes Gian Luigi Granato INAFPadova - 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 ...
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 ...
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Renaissance: Formation of the first light sources in the Universe after the Dark Ages PowerPoint PPT Presentation
Renaissance: Formation of the first light sources in the Universe after the Dark Ages - Quasars observed to z = 6 first ones must have formed in first Gyr ... First star and quasar formation limited to theory and simulation (with some ...
Quasars observed to z = 6 first ones must have formed in first Gyr ... First star and quasar formation limited to theory and simulation (with some ...
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Gravitational Wave Detection Using Pulsar Timing Current Status and Future Progress PowerPoint PPT Presentation
Gravitational Wave Detection Using Pulsar Timing Current Status and Future Progress - University of Texas at Brownsville. Collaborators. Dick Manchester. ATNF/CSIRO. Australia ... Teviet Creighton. Caltech. USA. John Armstrong. JPL. USA. Main Points ...
University of Texas at Brownsville. Collaborators. Dick Manchester. ATNF/CSIRO. Australia ... Teviet Creighton. Caltech. USA. John Armstrong. JPL. USA. Main Points ...
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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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