153 Qpos PPTs View free & download

QPOs and Nonlinear Pendulums PowerPoint PPT Presentation

QPOs and Nonlinear Pendulums - High frequency (kHz) QPOs lie in the range of ORBITAL FREQUENCIES of geodesics ... Relativistic precession model (Stella&Vietri 1998) ...

High frequency (kHz) QPOs lie in the range of ORBITAL FREQUENCIES of geodesics ... Relativistic precession model (Stella&Vietri 1998) ...

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HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL PowerPoint PPT Presentation

HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL - HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics, N.Novgorod)

HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics, N.Novgorod)

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Global MHD Simulations of State Transitions and QPOs in Black Hole Accretion Flows PowerPoint PPT Presentation

Global MHD Simulations of State Transitions and QPOs in Black Hole Accretion Flows - Global MHD Simulations of State Transitions and QPOs in Black Hole Accretion Flows ... Hardness Intensity Diagram. Power Spectrum. Belloni et al.(2006) fig.2 ...

Global MHD Simulations of State Transitions and QPOs in Black Hole Accretion Flows ... Hardness Intensity Diagram. Power Spectrum. Belloni et al.(2006) fig.2 ...

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Accreting Neutron Stars, Equations of State, and Gravitational Waves PowerPoint PPT Presentation

Accreting Neutron Stars, Equations of State, and Gravitational Waves - High Mass X-ray Binaries (Mc 1Mo) slow pulsars. often wind-fed. eg, Vela X-1 'Atoll' sources ... Various QPOs and peaked noise components for an Atoll source ...

High Mass X-ray Binaries (Mc 1Mo) slow pulsars. often wind-fed. eg, Vela X-1 'Atoll' sources ... Various QPOs and peaked noise components for an Atoll source ...

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Chapter 6 nuclear changes PowerPoint PPT Presentation

Chapter 6 nuclear changes - Copy chart 6-2 page 192. Exponential decay. Graph on page 290. Does the matter ... Sometimes: Quasi-periodic oscillations (QPOs) Sometimes: Radio-emitting jets ...

Copy chart 6-2 page 192. Exponential decay. Graph on page 290. Does the matter ... Sometimes: Quasi-periodic oscillations (QPOs) Sometimes: Radio-emitting jets ...

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QuasiPeriodic Oscillations in accretion onto compact objects PowerPoint PPT Presentation

QuasiPeriodic Oscillations in accretion onto compact objects - van der Klis, M. 2000, ARAA, 38:717-60 ... Atoll Sources. L~ (0.02-0.1) L_Edd ... atoll source. Z source. black hole candidate. kHz QPOs: Black Hole Candidates ...

van der Klis, M. 2000, ARAA, 38:717-60 ... Atoll Sources. L~ (0.02-0.1) L_Edd ... atoll source. Z source. black hole candidate. kHz QPOs: Black Hole Candidates ...

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Snmek 1 - 'Stella' Total precession 'Bursa' On the unity of black hole and neutron star kHz QPOs ... Stella, Bursa, total precession and disc-oscillation relation ...

'Stella' Total precession 'Bursa' On the unity of black hole and neutron star kHz QPOs ... Stella, Bursa, total precession and disc-oscillation relation ...

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Interpretation of HFQPOs as hydrodynamic disk modes near compact objects PowerPoint PPT Presentation

Interpretation of HFQPOs as hydrodynamic disk modes near compact objects - Hydrodynamic effects on the amplification and suppression of oscillatory modes ... disks is therefore a necessary first step to understand QPO phenomenology ...

Hydrodynamic effects on the amplification and suppression of oscillatory modes ... disks is therefore a necessary first step to understand QPO phenomenology ...

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PSCCUNY WELFARE FUND - Eligible for basic health coverage under the NYC Health Benefits Program ... Persons with : HIP-POS, Aetna QPOS, Aetna HMO, CIGNA or GHI-HMO will be ...

Eligible for basic health coverage under the NYC Health Benefits Program ... Persons with : HIP-POS, Aetna QPOS, Aetna HMO, CIGNA or GHI-HMO will be ...

Mass - Mass & Radius of Compact Objects Fastest pulsar and its stellar EOS CHENGMIN ZHANG National Astronomical Observatories Chinese Academy of Sciences, Beijing

Mass & Radius of Compact Objects Fastest pulsar and its stellar EOS CHENGMIN ZHANG National Astronomical Observatories Chinese Academy of Sciences, Beijing

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INPE Advanced Course on Compact Objects Course IV: Accretion Processes in Neutron Stars PowerPoint PPT Presentation

INPE Advanced Course on Compact Objects Course IV: Accretion Processes in Neutron Stars - INPE Advanced Course on Compact Objects Course IV: Accretion Processes in Neutron Stars & Black Holes Ron Remillard Kavli Center for Astrophysics and Space Research

INPE Advanced Course on Compact Objects Course IV: Accretion Processes in Neutron Stars & Black Holes Ron Remillard Kavli Center for Astrophysics and Space Research

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Black Holes: Observations Lecture 2: BHs in close binaries PowerPoint PPT Presentation

Black Holes: Observations Lecture 2: BHs in close binaries - Black Holes: Observations Lecture 2: BHs in close binaries Sergei Popov (SAI MSU) Plan of the lecture Reviews X-ray observations: Cyg X-1 X-ray novae X-ray nova light ...

Black Holes: Observations Lecture 2: BHs in close binaries Sergei Popov (SAI MSU) Plan of the lecture Reviews X-ray observations: Cyg X-1 X-ray novae X-ray nova light ...

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Slajd%201 - Analysing X-ray spectra from Beppo SAX authors found that strong wind from WR ... Type I bursts are observed in systems with highly eccentric orbits. ...

Analysing X-ray spectra from Beppo SAX authors found that strong wind from WR ... Type I bursts are observed in systems with highly eccentric orbits. ...

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Sn - Figs: from the collection of van der Klis, 2006. frequency. power. Sco X-1 ... Amplitude difference Dr = rL rU as it behaves in terms of the frequency ratio R ...

Figs: from the collection of van der Klis, 2006. frequency. power. Sco X-1 ... Amplitude difference Dr = rL rU as it behaves in terms of the frequency ratio R ...

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Nuclear Explosions on Rapidly Rotating Neutron Stars PowerPoint PPT Presentation

Nuclear Explosions on Rapidly Rotating Neutron Stars - Hydrodynamics of type-I bursts. Spitkovsky, L., Ushomirsky 02. L. ... Cooper & Narayan 06,07. Pros: 1. Coherence! 2. Fractional amplitude increases with energy ...

Hydrodynamics of type-I bursts. Spitkovsky, L., Ushomirsky 02. L. ... Cooper & Narayan 06,07. Pros: 1. Coherence! 2. Fractional amplitude increases with energy ...

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High Energy Universe Viewed Through Astrosat PowerPoint PPT Presentation

High Energy Universe Viewed Through Astrosat - High Energy Universe Viewed Through Astrosat P.C.Agrawal Tata Institute of Fundamental Research, Mumbai Talk at the Chandrayan Symposium at IMSc , Chennai , January 4 ...

High Energy Universe Viewed Through Astrosat P.C.Agrawal Tata Institute of Fundamental Research, Mumbai Talk at the Chandrayan Symposium at IMSc , Chennai , January 4 ...

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XIV%20Advanced%20School%20on%20Astrophysics%20Topic%20III:%20Observations%20of%20the%20Accretion%20Disks%20of%20Black%20Holes%20and%20Neutron%20Stars%20III.3:%20Accretion%20Disks%20of%20Non-Magnetic%20Neutron%20Stars - XIV Advanced School on Astrophysics Topic III: Observations of the Accretion Disks of Black Holes and Neutron Stars III.3: Accretion Disks of Non-Magnetic Neutron Stars

XIV Advanced School on Astrophysics Topic III: Observations of the Accretion Disks of Black Holes and Neutron Stars III.3: Accretion Disks of Non-Magnetic Neutron Stars

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Indian%20Astronomy%20Satellite%20Mission%20(ASTROSAT) PowerPoint PPT Presentation

Indian%20Astronomy%20Satellite%20Mission%20(ASTROSAT) - Tata Institute of Fundamental ... Mumbai, INDIA National Institutions ISRO, Bangalore TIFR, Mumbai IIA ... CAM with Holder Collimator CZT Top Housing CZT Bottom ...

Tata Institute of Fundamental ... Mumbai, INDIA National Institutions ISRO, Bangalore TIFR, Mumbai IIA ... CAM with Holder Collimator CZT Top Housing CZT Bottom ...

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Towards A unified model of Xray variability in Xray binaries and AGN PowerPoint PPT Presentation

Towards A unified model of Xray variability in Xray binaries and AGN - (Towards) A unified model of X-ray variability in X-ray binaries and AGN. Phil ... L(t) has a Gaussian distribution, so X(t) has a lognormal distribution...

(Towards) A unified model of X-ray variability in X-ray binaries and AGN. Phil ... L(t) has a Gaussian distribution, so X(t) has a lognormal distribution...

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Microsoft PowerPoint Tutorial PowerPoint PPT Presentation

Microsoft PowerPoint Tutorial - Title: Microsoft PowerPoint Tutorial Author: Clarkson University Last modified by: Saltiel Created Date: 7/25/2001 3:22:57 PM Document presentation format

Title: Microsoft PowerPoint Tutorial Author: Clarkson University Last modified by: Saltiel Created Date: 7/25/2001 3:22:57 PM Document presentation format

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Comments on John Rice PowerPoint PPT Presentation

Comments on John Rice - Title: PowerPoint Presentation Author: Jeffrey D. Scargle Last modified by: jeffrey Created Date: 6/10/2006 10:44:27 PM Document presentation format

Title: PowerPoint Presentation Author: Jeffrey D. Scargle Last modified by: jeffrey Created Date: 6/10/2006 10:44:27 PM Document presentation format

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Highspeed photometry of outbursting AM CVn stars PowerPoint PPT Presentation

Highspeed photometry of outbursting AM CVn stars - Three new AM CVns discovered recently all fall into the category ... `re-brightening' Maximum brightness: V ~ 15.0 mag (2004 outburst) ...

Three new AM CVns discovered recently all fall into the category ... `re-brightening' Maximum brightness: V ~ 15.0 mag (2004 outburst) ...

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X-ray binary jets: a.k.a. microquasars PowerPoint PPT Presentation

X-ray binary jets: a.k.a. microquasars - X-ray binary jets: a.k.a. microquasars Rob Fender (Southampton)

X-ray binary jets: a.k.a. microquasars Rob Fender (Southampton)

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Periodicities in variable stars: a few issues PowerPoint PPT Presentation

Periodicities in variable stars: a few issues - Periodicities in variable stars: a few issues Chris Koen Dept. Statistics University of the Western Cape

Periodicities in variable stars: a few issues Chris Koen Dept. Statistics University of the Western Cape

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40 Years of Mystery: Unravelling BZ UMa PowerPoint PPT Presentation

40 Years of Mystery: Unravelling BZ UMa - Porb = 0.0679d (Ringwald & Thorstenson, 1990) q= 0.2 (Jurcevic, Honeycutt, ... Dual-beam Imaging Polarimeter (DBIP) on UH 2.2m oN Mauna Kea (Masiero, Hodapp, ...

Porb = 0.0679d (Ringwald & Thorstenson, 1990) q= 0.2 (Jurcevic, Honeycutt, ... Dual-beam Imaging Polarimeter (DBIP) on UH 2.2m oN Mauna Kea (Masiero, Hodapp, ...

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Double feature: PowerPoint PPT Presentation

Double feature: - Double feature: Yuri Levin, Leiden. 1. The theory of fast oscillations ... Physics preliminaries: magnetic fields in non-resistive media. B. Field lines: ...

Double feature: Yuri Levin, Leiden. 1. The theory of fast oscillations ... Physics preliminaries: magnetic fields in non-resistive media. B. Field lines: ...

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Are there atoll/Z sources in HMXB? A rapid aperiodic timing analysis of 4 accreting X-ray pulsars in outburst Pablo Reig IESL, Foundation for Research - broad (zero-centred L) noise for low and high frequencies. peaked noise for intermediate frequencies. HMXB vs LMXB: differences. different topology ...

broad (zero-centred L) noise for low and high frequencies. peaked noise for intermediate frequencies. HMXB vs LMXB: differences. different topology ...

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High Energy Astrophysics: problems and expectations PowerPoint PPT Presentation

High Energy Astrophysics: problems and expectations - ... early universe (gamma ray bursts, X ray lines, optical and ... Intermediate mass black holes= ultraluminous X ray sources? ( or are they micro blazars? ...

... early universe (gamma ray bursts, X ray lines, optical and ... Intermediate mass black holes= ultraluminous X ray sources? ( or are they micro blazars? ...

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Thermonuclear bursts from slowly and rapidly accreting neutron stars PowerPoint PPT Presentation

Thermonuclear bursts from slowly and rapidly accreting neutron stars - Thermonuclear bursts from slowly and rapidly accreting neutron stars Manu Linares D. Chakrabarty, D. Altamirano, A. Cumming, L. Keek. V. Connaughton, P. Jenke, A ...

Thermonuclear bursts from slowly and rapidly accreting neutron stars Manu Linares D. Chakrabarty, D. Altamirano, A. Cumming, L. Keek. V. Connaughton, P. Jenke, A ...

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MICROQUASARS PowerPoint PPT Presentation

MICROQUASARS - LS 5039 has HESS counterpart 100 GeV (Aharonian et al. Science 2005) Both are massive stars in eccentric orbits. around compact objects of 4 M ...

LS 5039 has HESS counterpart 100 GeV (Aharonian et al. Science 2005) Both are massive stars in eccentric orbits. around compact objects of 4 M ...

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SUMMARY - SUMMARY PROBING STRONG GRAVITY IN AGN Kirpal Nandra Imperial College London

SUMMARY PROBING STRONG GRAVITY IN AGN Kirpal Nandra Imperial College London

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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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TIMING THE ACCRETION FLOW AROUND ACCRETING MILLISECOND PULSARS PowerPoint PPT Presentation

TIMING THE ACCRETION FLOW AROUND ACCRETING MILLISECOND PULSARS - AVERAGE SEPARATION: 205 -6 Hz. PULSE: 191 Hz. Michiel's talk. 4U 1728-34. XTE J1807-294 ... Are break frequency and accretion rate correlated? 4U 1608-52 (AMPs ...

AVERAGE SEPARATION: 205 -6 Hz. PULSE: 191 Hz. Michiel's talk. 4U 1728-34. XTE J1807-294 ... Are break frequency and accretion rate correlated? 4U 1608-52 (AMPs ...

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Comments on John Rices paper PowerPoint PPT Presentation

Comments on John Rices paper - This paper should be quite accessible to astronomers: ... AIP Conference Proceedings, ed. Robert L. Fry. http://proceedings.aip.org/ (volume617) ...

This paper should be quite accessible to astronomers: ... AIP Conference Proceedings, ed. Robert L. Fry. http://proceedings.aip.org/ (volume617) ...

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ArgosX: Advances in WideAngle Xray Instrumentation PowerPoint PPT Presentation

ArgosX: Advances in WideAngle Xray Instrumentation - Argos-X simulated spectra from a BH binary (Jon Miller RR) ... Science Objectives for Argos-X. Timing Themes for X-ray Binaries ...

Argos-X simulated spectra from a BH binary (Jon Miller RR) ... Science Objectives for Argos-X. Timing Themes for X-ray Binaries ...

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Microsoft PowerPoint Tutorial - ... cascading with 2D nonlinear photonic crystals Methods for double phase matching DPM with ... QPM - quasi phase matching ... Equation 3.0 Microsoft ...

... cascading with 2D nonlinear photonic crystals Methods for double phase matching DPM with ... QPM - quasi phase matching ... Equation 3.0 Microsoft ...

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Accretion in Binaries PowerPoint PPT Presentation

Accretion in Binaries - Burst Energetics ... If Type I bursts are due to thermal nuclear processes, a ... Burst oscillations and coherent persistent oscillations in SAX J1808.4-3658 are ...

Burst Energetics ... If Type I bursts are due to thermal nuclear processes, a ... Burst oscillations and coherent persistent oscillations in SAX J1808.4-3658 are ...

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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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High Speed, High Precision Photometry with Orthogonal Transfer CCDs PowerPoint PPT Presentation

High Speed, High Precision Photometry with Orthogonal Transfer CCDs - OPTIC is the prototype OTCCD camera. OPTIC contains two ... Asteroid FC5 2003. V~17, Both are 200 sec exposures. S/N ~6 times higher. High Speed (Video) Mode ...

OPTIC is the prototype OTCCD camera. OPTIC contains two ... Asteroid FC5 2003. V~17, Both are 200 sec exposures. S/N ~6 times higher. High Speed (Video) Mode ...

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Gefangen im Wirbel aus Raum und Zeit - Rotierende Schwarze L PowerPoint PPT Presentation

Gefangen im Wirbel aus Raum und Zeit - Rotierende Schwarze L - Gefangen im Wirbel aus Raum und Zeit - Rotierende Schwarze L cher 08.12.2004 AK Astronomie Universit t Stuttgart Andreas M ller Theoriegruppe Landessternwarte ...

Gefangen im Wirbel aus Raum und Zeit - Rotierende Schwarze L cher 08.12.2004 AK Astronomie Universit t Stuttgart Andreas M ller Theoriegruppe Landessternwarte ...

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Ultraluminous Xray sources: highlights on NGC1313 X2 and M82 X1 PowerPoint PPT Presentation

Ultraluminous Xray sources: highlights on NGC1313 X2 and M82 X1 - Ultraluminous X-ray sources: highlights on NGC1313 X-2 and M82 X-1 ... NGC1313 is a nearby spiral galaxy hosting two ULXs, NGC1313 X-1 and X-2, and the ...

Ultraluminous X-ray sources: highlights on NGC1313 X-2 and M82 X-1 ... NGC1313 is a nearby spiral galaxy hosting two ULXs, NGC1313 X-1 and X-2, and the ...

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Variables%20Cataclysmiques%20:%20Accr PowerPoint PPT Presentation

Variables%20Cataclysmiques%20:%20Accr - Si volution jointe des 2 toiles (non capture), le temps d' volution ... Ajustement spectral : Plasma mission (mekal / continu raies) -si temp rature uniforme T ...

Si volution jointe des 2 toiles (non capture), le temps d' volution ... Ajustement spectral : Plasma mission (mekal / continu raies) -si temp rature uniforme T ...

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Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode (presentation mode). - Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode

Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode

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Is the Formation of Relativistic Jets a Fiction 30 Years BZ Mechanism PowerPoint PPT Presentation

Is the Formation of Relativistic Jets a Fiction 30 Years BZ Mechanism - ... approach understood: rotating MS, plasma injection, acceleration and collimation. Correlation between X-ray states and Jet production (in micro-quasars, RXTE) ...

... approach understood: rotating MS, plasma injection, acceleration and collimation. Correlation between X-ray states and Jet production (in micro-quasars, RXTE) ...

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Neutron Stars and Black Holes PowerPoint PPT Presentation

Neutron Stars and Black Holes - 0 Chapter 14 Neutron Stars and Black Holes

0 Chapter 14 Neutron Stars and Black Holes

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Isolated Neutron Stars: From the Surface to the Interiors PowerPoint PPT Presentation

Isolated Neutron Stars: From the Surface to the Interiors - New NS atmosphere/surface models [Pons, Mori, Ho, Lai] ... field possibly nondipolar, with a toroidal component [Pons, Zane, Ruderman, Page] ...

New NS atmosphere/surface models [Pons, Mori, Ho, Lai] ... field possibly nondipolar, with a toroidal component [Pons, Zane, Ruderman, Page] ...

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Probing the neutron star physics with accreting neutron stars (part 2) PowerPoint PPT Presentation

Probing the neutron star physics with accreting neutron stars (part 2) - Probing the neutron star physics with accreting neutron stars (part 2) ... Use of three wonderful satellites: Chandra, XMM-Newton, RXTE. Outburst vs. quiescence ...

Probing the neutron star physics with accreting neutron stars (part 2) ... Use of three wonderful satellites: Chandra, XMM-Newton, RXTE. Outburst vs. quiescence ...

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New Results From Pulse Shape Models for the ms Pulsar SAX J1808.4-3658 PowerPoint PPT Presentation

New Results From Pulse Shape Models for the ms Pulsar SAX J1808.4-3658 - How pulse shape modeling constrains Mass and Radius. Why millisecond X-ray pulsars are good candidates. New results for SAX J1808 ...

How pulse shape modeling constrains Mass and Radius. Why millisecond X-ray pulsars are good candidates. New results for SAX J1808 ...

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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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The Hard X-ray Modulation Telescope (HXMT) PowerPoint PPT Presentation

The Hard X-ray Modulation Telescope (HXMT) - The Hard X-ray Modulation Telescope (HXMT) Fangjun Lu (Institute of High Energy Physics, Chinese Academy of Sciences) On behalf of the HXMT group

The Hard X-ray Modulation Telescope (HXMT) Fangjun Lu (Institute of High Energy Physics, Chinese Academy of Sciences) On behalf of the HXMT group

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Sequential Logic PowerPoint PPT Presentation

Sequential Logic - Sequential Circuits Simple circuits with feedback Latches Edge-triggered flip-flops Timing Methodologies Cascading flip-flops for proper operation

Sequential Circuits Simple circuits with feedback Latches Edge-triggered flip-flops Timing Methodologies Cascading flip-flops for proper operation

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X-ray spectral index correlations vs mass accretion rate in black hole binaries in their different spectral states. Theory vs observations PowerPoint PPT Presentation

X-ray spectral index correlations vs mass accretion rate in black hole binaries in their different spectral states. Theory vs observations - Title: PowerPoint Presentation Author: Lev Titarchuk Last modified by: Lev Titarchuk Created Date: 6/28/2006 9:16:59 AM Document presentation format

Title: PowerPoint Presentation Author: Lev Titarchuk Last modified by: Lev Titarchuk Created Date: 6/28/2006 9:16:59 AM Document presentation format

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Black Holes, Gravity to the Max PowerPoint PPT Presentation

Black Holes, Gravity to the Max - Black Holes, Gravity to the Max By Dr. Harold Williams of Montgomery College Planetarium http://montgomerycollege.edu/Departments/planet/ Given in the planetarium ...

Black Holes, Gravity to the Max By Dr. Harold Williams of Montgomery College Planetarium http://montgomerycollege.edu/Departments/planet/ Given in the planetarium ...

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Neutron Stars 4: Magnetism PowerPoint PPT Presentation

Neutron Stars 4: Magnetism - Neutron Stars 4: Magnetism Andreas Reisenegger ESO Visiting Scientist Associate Professor, Pontificia Universidad Cat lica de Chile

Neutron Stars 4: Magnetism Andreas Reisenegger ESO Visiting Scientist Associate Professor, Pontificia Universidad Cat lica de Chile

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Pr - ... 5039: from radio and GeV emission from EGRET (Paredes et al. 2000) to VHE gamma ... from radio and GeV emission from EGRET (Paredes et al. 2000) to VHE ...

... 5039: from radio and GeV emission from EGRET (Paredes et al. 2000) to VHE gamma ... from radio and GeV emission from EGRET (Paredes et al. 2000) to VHE ...

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The Why - Eclipses (10s min days) Accretion disks (~ms years) Transients (X-ray novae) ... Distributed as 2 with 2 degrees of freedom (d.o.f.) for the Leahy normalization ...

Eclipses (10s min days) Accretion disks (~ms years) Transients (X-ray novae) ... Distributed as 2 with 2 degrees of freedom (d.o.f.) for the Leahy normalization ...

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Qpos PowerPoint PPT Presentations