Begelman PowerPoint PPT Presentations

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Moderator: Mitch Begelman PowerPoint PPT Presentation
Moderator: Mitch Begelman - ... of the jet with the cluster gas as a calorimeter (some progress already made! ... the X-ray calorimeter on NeXT, but poor angular resolution - must be used in ...
... of the jet with the cluster gas as a calorimeter (some progress already made! ... the X-ray calorimeter on NeXT, but poor angular resolution - must be used in ...
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Mitch Begelman PowerPoint PPT Presentation
Mitch Begelman - Mitch Begelman
Mitch Begelman
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Mitch Begelman PowerPoint PPT Presentation
Mitch Begelman - Depends on relative speed but not location of sources. For ... Consider continuously glowing blob, moving almost directly toward you at. 0.8c. 0.8 lt-day ...
Depends on relative speed but not location of sources. For ... Consider continuously glowing blob, moving almost directly toward you at. 0.8c. 0.8 lt-day ...
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Mitch Begelman PowerPoint PPT Presentation
Mitch Begelman - Mitch Begelman. JILA, University of Colorado. FORMATION AND ... YOU'VE GOT TO BE KIDDING. QUASISTAR PROPERTIES. Mass m* (M ) increases with time. Core with ...
Mitch Begelman. JILA, University of Colorado. FORMATION AND ... YOU'VE GOT TO BE KIDDING. QUASISTAR PROPERTIES. Mass m* (M ) increases with time. Core with ...
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Mark Begelman and Keith Ridenour's Studio Attract Famous Musicians. PowerPoint PPT Presentation
Mark Begelman and Keith Ridenour's Studio Attract Famous Musicians. - 1888PressRelease - Markee Music by Mark Begelman and Keith Ridenour continues it's dominance in Florida as the best place to record music.
1888PressRelease - Markee Music by Mark Begelman and Keith Ridenour continues it's dominance in Florida as the best place to record music.
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Evidence for UHECR Acceleration from Fermi Observations of AGNs and GRBs PowerPoint PPT Presentation
Evidence for UHECR Acceleration from Fermi Observations of AGNs and GRBs - 1. Evidence for UHECR Acceleration from Fermi Observations of AGNs and GRBs ... Cocoon dynamics (Begelman and Cioffi 1989 for Cyg A) ...
1. Evidence for UHECR Acceleration from Fermi Observations of AGNs and GRBs ... Cocoon dynamics (Begelman and Cioffi 1989 for Cyg A) ...
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Aim of this talk PowerPoint PPT Presentation
Aim of this talk - Blazars: basic picture. Sikora, Begelman & Rees (1994) Theorists claims that the size of ... Which one's responsible for the X-ray variability? Central engine ...
Blazars: basic picture. Sikora, Begelman & Rees (1994) Theorists claims that the size of ... Which one's responsible for the X-ray variability? Central engine ...
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Xray Astronomy in the Next Decade 90% of the matter in the universe can only be seen via xray observ PowerPoint PPT Presentation
Xray Astronomy in the Next Decade 90% of the matter in the universe can only be seen via xray observ - X-ray Astronomy in the Next Decade. 90% of the matter in the universe can only be ... M.Begelman, TJ Cox, D. Croton, T. DiMatteo, I. George, C. Martin, J. Ostriker, V. ...
X-ray Astronomy in the Next Decade. 90% of the matter in the universe can only be ... M.Begelman, TJ Cox, D. Croton, T. DiMatteo, I. George, C. Martin, J. Ostriker, V. ...
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Markos Georganopoulos University of Maryland Baltimore County PowerPoint PPT Presentation
Markos Georganopoulos University of Maryland Baltimore County - Title: Markos Georganopoulos1,2 Eric Perlman1 Demosthenes Kazanas2 Brian Wingert1 1: UMBC 2:NASA/GSFC Author: Markos Last modified by
Title: Markos Georganopoulos1,2 Eric Perlman1 Demosthenes Kazanas2 Brian Wingert1 1: UMBC 2:NASA/GSFC Author: Markos Last modified by
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On the convective instability of hot radiative accretion flow PowerPoint PPT Presentation
On the convective instability of hot radiative accretion flow - ... Black hole growth Black hole spin evolution Previous works neglect radiative cooling Radiation is often very important, ... entropy increases inward ...
... Black hole growth Black hole spin evolution Previous works neglect radiative cooling Radiation is often very important, ... entropy increases inward ...
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Relaxation of Pulsar Wind Nebula via Current-Driven Kink Instability PowerPoint PPT Presentation
Relaxation of Pulsar Wind Nebula via Current-Driven Kink Instability - Yosuke Mizuno ( ) Institute of Astronomy National Tsing-Hua University Collaborators Y. Lyubarsky (Ben-Gurion Univ), K.-I. Nishikawa (NSSTC/UAH), P. E ...
Yosuke Mizuno ( ) Institute of Astronomy National Tsing-Hua University Collaborators Y. Lyubarsky (Ben-Gurion Univ), K.-I. Nishikawa (NSSTC/UAH), P. E ...
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Jet-Disk Connection in AGNs PowerPoint PPT Presentation
Jet-Disk Connection in AGNs - a prominent accretion disk in the low-hard state of the black hole candidate: Truncated disk? There are always OUTLIERS! Accretion Mode in BL Lacs+RLQs (Wang ...
a prominent accretion disk in the low-hard state of the black hole candidate: Truncated disk? There are always OUTLIERS! Accretion Mode in BL Lacs+RLQs (Wang ...
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What Can Transients Reveal about Massive Black Hole Assembly PowerPoint PPT Presentation
What Can Transients Reveal about Massive Black Hole Assembly - GG Tau: Potter/Hawaii/Gemini/AURA/NSF. 07/11/06. 10. Gas around Binary Black Holes: Alignment ... initial surface density profile. surface density after ...
GG Tau: Potter/Hawaii/Gemini/AURA/NSF. 07/11/06. 10. Gas around Binary Black Holes: Alignment ... initial surface density profile. surface density after ...
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A Heino-Centric View of the History of Galactic Center Theory PowerPoint PPT Presentation
A Heino-Centric View of the History of Galactic Center Theory - A Heino-Centric View of the History of Galactic Center Theory ... Spin, precession and variability of Sgr A*. Linear Polarization images near the event horizon ...
A Heino-Centric View of the History of Galactic Center Theory ... Spin, precession and variability of Sgr A*. Linear Polarization images near the event horizon ...
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ADIOS Revisited PowerPoint PPT Presentation
ADIOS Revisited - 456789:CDEFGHIJSTUVWXYZcdefghijstuvwxyz rl e cC nuu ? nNSsz GpSs tFTO ... ( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c ( c( c ...
456789:CDEFGHIJSTUVWXYZcdefghijstuvwxyz rl e cC nuu ? nNSsz GpSs tFTO ... ( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c( c ( c( c ...
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Trapping of Magnetic Flux by a Black Hole Accretion Disk PowerPoint PPT Presentation
Trapping of Magnetic Flux by a Black Hole Accretion Disk - 0) Importance of the field threading the black hole ... Geometry of field is governed by Maxwell's eqns. dragging dominates diffusion ...
0) Importance of the field threading the black hole ... Geometry of field is governed by Maxwell's eqns. dragging dominates diffusion ...
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Amir Levinson PowerPoint PPT Presentation
Amir Levinson - Title: No Slide Title Author: Amir Levinson Last modified by: Admin amir Created Date: 8/26/2002 1:03:38 PM Document presentation format: Pr sentation l' cran (4:3)
Title: No Slide Title Author: Amir Levinson Last modified by: Admin amir Created Date: 8/26/2002 1:03:38 PM Document presentation format: Pr sentation l' cran (4:3)
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Linear and Circular Polarization from Sagittarius A* PowerPoint PPT Presentation
Linear and Circular Polarization from Sagittarius A* - Mdot 10-5 M_sun y-1. Bandwidth depolarization. RM 5 x 106 rad m-2. Mdot 10-3 M_sun y-1. Summary. Polarization is a unique probe of Sgr A ...
Mdot 10-5 M_sun y-1. Bandwidth depolarization. RM 5 x 106 rad m-2. Mdot 10-3 M_sun y-1. Summary. Polarization is a unique probe of Sgr A ...
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Gamma-ray emission from AGN PowerPoint PPT Presentation
Gamma-ray emission from AGN - Gamma-ray emission from AGN Qinghuan Luo School of Physics, University of Sydney
Gamma-ray emission from AGN Qinghuan Luo School of Physics, University of Sydney
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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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Blazar Variability PowerPoint PPT Presentation
Blazar Variability - Blazar Variability
Blazar Variability
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EXPLOSION OF VERY MASSIVE STARS AND THE ORIGIN OF INTERMEDIATE MASS BLACK HOLES PowerPoint PPT Presentation
EXPLOSION OF VERY MASSIVE STARS AND THE ORIGIN OF INTERMEDIATE MASS BLACK HOLES - I. INTRODUCTION. II. OUR RECENT RESEARCH. III. SUMMARY/CONCLUSION. 3 ... consistent with IMBH mass (iii) Abundance pattern ...consistent with M82 gas, ICM, IGM ...
I. INTRODUCTION. II. OUR RECENT RESEARCH. III. SUMMARY/CONCLUSION. 3 ... consistent with IMBH mass (iii) Abundance pattern ...consistent with M82 gas, ICM, IGM ...
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Observational Evidence of Black Holes PowerPoint PPT Presentation
Observational Evidence of Black Holes - Observational Evidence of Black Holes
Observational Evidence of Black Holes
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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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The interaction between AGN and the ICM PowerPoint PPT Presentation
The interaction between AGN and the ICM - The interaction between AGN and the ICM
The interaction between AGN and the ICM
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Black Hole Accretion PowerPoint PPT Presentation
Black Hole Accretion - Advection-Dominated Accretion Flow, ADAF (Ichimaru 1977; Narayan & Yi 1994, 1995; ... We suggest that advection-dominated accretion may provide an explanation for ...
Advection-Dominated Accretion Flow, ADAF (Ichimaru 1977; Narayan & Yi 1994, 1995; ... We suggest that advection-dominated accretion may provide an explanation for ...
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Mixing Layer Theory and a Numerical Search for High Ions PowerPoint PPT Presentation
Mixing Layer Theory and a Numerical Search for High Ions - Hot gas dissipates energy through an interface layer into a ... Reflection prevents energy ... May2003Instead, said astronomer Barry Welsh of UC Berkeley's ...
Hot gas dissipates energy through an interface layer into a ... Reflection prevents energy ... May2003Instead, said astronomer Barry Welsh of UC Berkeley's ...
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Elena Belsole PowerPoint PPT Presentation
Elena Belsole - The new picture from Chandra and XMM. Conclusions. Future prospects. Elena Belsole ... X-ray emission traces the hot gas component. ...
The new picture from Chandra and XMM. Conclusions. Future prospects. Elena Belsole ... X-ray emission traces the hot gas component. ...
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Short-Duration Gamma-Ray Burst Central Engines PowerPoint PPT Presentation
Short-Duration Gamma-Ray Burst Central Engines - (Rosswog 07; Faber 06; Lee 09) a. r - Process Heating (not included in present simulations! ... NS Matter A ~ 100 Nuclei Free Neutrons (Lattimer 77; Meyer 89) ...
(Rosswog 07; Faber 06; Lee 09) a. r - Process Heating (not included in present simulations! ... NS Matter A ~ 100 Nuclei Free Neutrons (Lattimer 77; Meyer 89) ...
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Probing Accretion and Spacetime with Black Hole Binaries PowerPoint PPT Presentation
Probing Accretion and Spacetime with Black Hole Binaries - Stellar Atmospheres: Disk Annuli vs. Stellar Envelopes ... Annuli are determined by, Teff, Q (where g=Q z), , the composition, and the ...
Stellar Atmospheres: Disk Annuli vs. Stellar Envelopes ... Annuli are determined by, Teff, Q (where g=Q z), , the composition, and the ...
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Distribution of the ISM PowerPoint PPT Presentation
Distribution of the ISM - Measurement of halo HI done by comparing Lya absorption against high-Z stars to ... Primordial extragalactic gas, halo supernovae, galactic fountain ...
Measurement of halo HI done by comparing Lya absorption against high-Z stars to ... Primordial extragalactic gas, halo supernovae, galactic fountain ...
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Advection-dominated Accretion: PowerPoint PPT Presentation
Advection-dominated Accretion: - Advection-dominated Accretion: From Sgr A* to Other Low-Luminosity AGNs Feng Yuan Shanghai Astronomical Observatory
Advection-dominated Accretion: From Sgr A* to Other Low-Luminosity AGNs Feng Yuan Shanghai Astronomical Observatory
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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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THE ROLE OF BLACK HOLES IN GALAXY EVOLUTION PowerPoint PPT Presentation
THE ROLE OF BLACK HOLES IN GALAXY EVOLUTION - Volker Springel, Lars Hernquist, Phil Hopkins, Brant Robertson, TJ Cox. OUTLINE: BHs in Isolated Galaxies & Mergers - BHs galaxy formation. BHs in Cosmological ...
Volker Springel, Lars Hernquist, Phil Hopkins, Brant Robertson, TJ Cox. OUTLINE: BHs in Isolated Galaxies & Mergers - BHs galaxy formation. BHs in Cosmological ...
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ULX accretion state PowerPoint PPT Presentation
ULX accretion state - D Swartz (MSFC), A Goncalves (Paris-M), R Mushotzky, T ... ULXs may have a persistently. super-Edd accretion rate. High/soft. Very high. ultraluminous ...
D Swartz (MSFC), A Goncalves (Paris-M), R Mushotzky, T ... ULXs may have a persistently. super-Edd accretion rate. High/soft. Very high. ultraluminous ...
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Modeling Supercritical Accretion Flow Shin Mineshige (Kyoto) PowerPoint PPT Presentation
Modeling Supercritical Accretion Flow Shin Mineshige (Kyoto) - Title: Author: Shin Mineshige Last modified by: minesige Created Date: 9/18/2000 10:11:14 AM Document presentation format
Title: Author: Shin Mineshige Last modified by: minesige Created Date: 9/18/2000 10:11:14 AM Document presentation format
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Gamma-Ray Burst Early Afterglows PowerPoint PPT Presentation
Gamma-Ray Burst Early Afterglows - Gamma-Ray Burst Early Afterglows. Bing Zhang. Physics Department. University of Nevada, Las Vegas ... gamma-ray. UV/opt/IR/radio. Why is the early afterglow ...
Gamma-Ray Burst Early Afterglows. Bing Zhang. Physics Department. University of Nevada, Las Vegas ... gamma-ray. UV/opt/IR/radio. Why is the early afterglow ...
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Relativistic reconnection PowerPoint PPT Presentation
Relativistic reconnection - Total dissipation of alternating fields at the ... Bow shocks in binary pulsars at. Dissipation at shocks in AGNs: Levinson ... Luo & Melrose 2006 ...
Total dissipation of alternating fields at the ... Bow shocks in binary pulsars at. Dissipation at shocks in AGNs: Levinson ... Luo & Melrose 2006 ...
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AGN Feedback Heating in Clusters of Galaxies PowerPoint PPT Presentation
AGN Feedback Heating in Clusters of Galaxies - why AGN feedback in Galaxy Clusters? Heating the ICM -- Conduction vs ... Chandra image of Hydra A. For review papers, see. Fabian 1994. Peterson & Fabian 2006 ...
why AGN feedback in Galaxy Clusters? Heating the ICM -- Conduction vs ... Chandra image of Hydra A. For review papers, see. Fabian 1994. Peterson & Fabian 2006 ...
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OneDimensional Accretion Disk Model with Inflow PowerPoint PPT Presentation
OneDimensional Accretion Disk Model with Inflow - The thin accretion disk models describes a cooling-dominated flow in which the ... model provides the picture of how gases flow near the vicinity of a black hole ...
The thin accretion disk models describes a cooling-dominated flow in which the ... model provides the picture of how gases flow near the vicinity of a black hole ...
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Structure PowerPoint PPT Presentation
Structure - Limb Brightening of the Image a rapid transition an 'overshoot' ... Hydro-simulation: more limb brightening slightly faster transition larger overshoot ...
Limb Brightening of the Image a rapid transition an 'overshoot' ... Hydro-simulation: more limb brightening slightly faster transition larger overshoot ...
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PULSAR WIND NEBULAE FROM RADIO TO XRAYS PowerPoint PPT Presentation
PULSAR WIND NEBULAE FROM RADIO TO XRAYS - Radio-to-X-ray diagnostics composition, energy transport, magnetic field geometry ... Example: The Mouse (Gaensler et al. 03) Radio X-ray synchrotron tails ...
Radio-to-X-ray diagnostics composition, energy transport, magnetic field geometry ... Example: The Mouse (Gaensler et al. 03) Radio X-ray synchrotron tails ...
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Gamma Rays from Accreting Black Holes PowerPoint PPT Presentation
Gamma Rays from Accreting Black Holes - Gamma Ray Bursts? 1 ix 05. GLAST GC Meeting. 3. Traditional Disks are: ... X. Can you measure the toroidal field pattern? Even Parity. Odd Parity. Mixed Parity ...
Gamma Ray Bursts? 1 ix 05. GLAST GC Meeting. 3. Traditional Disks are: ... X. Can you measure the toroidal field pattern? Even Parity. Odd Parity. Mixed Parity ...
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Location of the TEVemitting region in PKS 2155304 PowerPoint PPT Presentation
Location of the TEVemitting region in PKS 2155304 - Stefan Wagner. Landessternwarte. University of Heidelberg. Variability of PKS 2155-304 ... If the emitting region is close to the black hole then ...
Stefan Wagner. Landessternwarte. University of Heidelberg. Variability of PKS 2155-304 ... If the emitting region is close to the black hole then ...
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Mixing Layer Theory and a Numerical Search for High Ions PowerPoint PPT Presentation
Mixing Layer Theory and a Numerical Search for High Ions - Hot gas dissipates energy through an interface layer into a colder ISM phase. ... cavities and tunnels, analogous to the holes in a sponge, were created ...
Hot gas dissipates energy through an interface layer into a colder ISM phase. ... cavities and tunnels, analogous to the holes in a sponge, were created ...
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Relativistic jets in Active galactic nuclei PowerPoint PPT Presentation
Relativistic jets in Active galactic nuclei - Collaborator: Hiroshi Nagai (NAOJ) and Motoki Kino (JAXA) ... e.g., van Brreugel, Miley & Heckman 1984. 2.Youth scenario. e.g., Phillips & Mutel 1982 ...
Collaborator: Hiroshi Nagai (NAOJ) and Motoki Kino (JAXA) ... e.g., van Brreugel, Miley & Heckman 1984. 2.Youth scenario. e.g., Phillips & Mutel 1982 ...
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Shock acceleration models personal review PowerPoint PPT Presentation
Shock acceleration models personal review - Shock acceleration models personal review
Shock acceleration models personal review
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Helical MagnetoRotational Instability and Issues in Astrophysical Jets PowerPoint PPT Presentation
Helical MagnetoRotational Instability and Issues in Astrophysical Jets - but jets are already prone to several vigorous instabilities. pinch, kink, Kelvin-Helmholtz, ... Astrophysical jets & outflows' ...
but jets are already prone to several vigorous instabilities. pinch, kink, Kelvin-Helmholtz, ... Astrophysical jets & outflows' ...
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RadiationDominated Accretion Disks PowerPoint PPT Presentation
RadiationDominated Accretion Disks - Shakura-Sunyaev Picture. Radiation-MHD Equations. Heating. Cooling. X-Ray Reflection. Summary ... Effects on X-Ray Reflection Variability. Assumptions tested: ...
Shakura-Sunyaev Picture. Radiation-MHD Equations. Heating. Cooling. X-Ray Reflection. Summary ... Effects on X-Ray Reflection Variability. Assumptions tested: ...
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Particle acceleration in Pulsar Wind Nebulae PowerPoint PPT Presentation
Particle acceleration in Pulsar Wind Nebulae - Resonant cyclotron absorption in ion doped plasma (Hoshino et al 92, Amato ... RCA of ion cyclotron waves works effectively as an acceleration mechanism for ...
Resonant cyclotron absorption in ion doped plasma (Hoshino et al 92, Amato ... RCA of ion cyclotron waves works effectively as an acceleration mechanism for ...
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Extragalactic Jets: Theory and Observation from Radio to Gamma Ray PowerPoint PPT Presentation
Extragalactic Jets: Theory and Observation from Radio to Gamma Ray - a candidate: 1855 37 (Giroletti 05) 1855 37: a jet turning off? 1855 37 ... Tsyn ~ 105-106 yr. vadv, syn c. consistent with slow/ceased advance in the ...
a candidate: 1855 37 (Giroletti 05) 1855 37: a jet turning off? 1855 37 ... Tsyn ~ 105-106 yr. vadv, syn c. consistent with slow/ceased advance in the ...
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The Hydrodynamics of Galaxy and MBH formation: Z,3 No early BHBH Mergers Stirling Colgate, Nathan Cu PowerPoint PPT Presentation
The Hydrodynamics of Galaxy and MBH formation: Z,3 No early BHBH Mergers Stirling Colgate, Nathan Cu - 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 ...
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 ...
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Ultraluminous X-ray Sources PowerPoint PPT Presentation
Ultraluminous X-ray Sources - Title: PowerPoint Presentation Author: Tim Roberts Last modified by: Martin Ward Created Date: 11/13/2000 10:42:03 AM Document presentation format
Title: PowerPoint Presentation Author: Tim Roberts Last modified by: Martin Ward Created Date: 11/13/2000 10:42:03 AM Document presentation format
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OneDimensional Accretion Disk Model with Inflow Outflow PowerPoint PPT Presentation
OneDimensional Accretion Disk Model with Inflow Outflow - (1) Models, (2) Descriptions, and (3) Flows ... Global models of thin accretion disk developed ... picture of how gases flow near the vicinity of a black hole ...
(1) Models, (2) Descriptions, and (3) Flows ... Global models of thin accretion disk developed ... picture of how gases flow near the vicinity of a black hole ...
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