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Excitation of the Neutron Star fmode in LMXBs PowerPoint PPT Presentation
Excitation of the Neutron Star fmode in LMXBs - Excitation of the Neutron Star f-mode in LMXBs. J. C. N. de Araujo, O. D. Miranda & O. D. Aguiar ... the glitch phenomenon (see de Araujo, Miranda & Aguiar 2005) ...
Excitation of the Neutron Star f-mode in LMXBs. J. C. N. de Araujo, O. D. Miranda & O. D. Aguiar ... the glitch phenomenon (see de Araujo, Miranda & Aguiar 2005) ...
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GRAVITATIONAL WAVES FROM ACCRETING NS PowerPoint PPT Presentation
GRAVITATIONAL WAVES FROM ACCRETING NS - Precession & superfluid circulation. NS SPINS IN LMXBs ... Precession damped: e3 W , no X-ray pulses, GW at 2f only (if triaxial) Excitation ...
Precession & superfluid circulation. NS SPINS IN LMXBs ... Precession damped: e3 W , no X-ray pulses, GW at 2f only (if triaxial) Excitation ...
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Evolution of X-ray Binaries and the Formation of Binary Pulsars PowerPoint PPT Presentation
Evolution of X-ray Binaries and the Formation of Binary Pulsars - Title: PowerPoint Presentation Last modified by: AAA Created Date: 1/1/1601 12:00:00 AM Document presentation format: Other titles
Title: PowerPoint Presentation Last modified by: AAA Created Date: 1/1/1601 12:00:00 AM Document presentation format: Other titles
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Populations of bright compact sources in galaxies PowerPoint PPT Presentation
Populations of bright compact sources in galaxies - Roche lobe overflow. Roche lobe overflow. stellar evolution. SN explosion ... LMXB - Roche-lobe overflow 'true' ULXs are associated with star-formation ...
Roche lobe overflow. Roche lobe overflow. stellar evolution. SN explosion ... LMXB - Roche-lobe overflow 'true' ULXs are associated with star-formation ...
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Philip J' Humphrey UC Irvine PowerPoint PPT Presentation
Philip J' Humphrey UC Irvine - Sample of 19 early-type galaxies from Chandra archive ... Omits very young systems. LMXB luminosity evolution with age. A simple evolutionary model ...
Sample of 19 early-type galaxies from Chandra archive ... Omits very young systems. LMXB luminosity evolution with age. A simple evolutionary model ...
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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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How LIGO searches are affected by theory PowerPoint PPT Presentation
How LIGO searches are affected by theory - Depends on what 'neutron' star is made of (how much is solid) ... not if perpendicular instability drives axes perpendicular (P. Jones 1970s) ...
Depends on what 'neutron' star is made of (how much is solid) ... not if perpendicular instability drives axes perpendicular (P. Jones 1970s) ...
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INSTABILITIES OF ROTATING RELATIVISTIC STARS PowerPoint PPT Presentation
INSTABILITIES OF ROTATING RELATIVISTIC STARS - INSTABILITIES OF ROTATING RELATIVISTIC STARS John Friedman University of Wisconsin-Milwaukee Center for Gravitation and Cosmology
INSTABILITIES OF ROTATING RELATIVISTIC STARS John Friedman University of Wisconsin-Milwaukee Center for Gravitation and Cosmology
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X-ray binaries and CXB PowerPoint PPT Presentation
X-ray binaries and CXB - Xray binaries and CXB
Xray binaries and CXB
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Mass PowerPoint PPT Presentation
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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Sn PowerPoint PPT Presentation
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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Accretion Power in Astrophysics PowerPoint PPT Presentation
Accretion Power in Astrophysics - Accretion Power in Astrophysics Andrew King Theoretical Astrophysics Group, University of Leicester, UK Accreting Black Holes in a Nearby Galaxy (M101) Accreting ...
Accretion Power in Astrophysics Andrew King Theoretical Astrophysics Group, University of Leicester, UK Accreting Black Holes in a Nearby Galaxy (M101) Accreting ...
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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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Neutron Star Model Atmospheres PowerPoint PPT Presentation
Neutron Star Model Atmospheres - Identification of gravitationally redshifted spectral lines ... NS atmospheres to compute cyclotron absorption lines and absorption by vacuum resonance opacity. ...
Identification of gravitationally redshifted spectral lines ... NS atmospheres to compute cyclotron absorption lines and absorption by vacuum resonance opacity. ...
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Interactions between gravitational waves and photon astronomy (periodic signals) PowerPoint PPT Presentation
Interactions between gravitational waves and photon astronomy (periodic signals) - Photon astronomy sets indirect upper limits on GW - milestones for sensitivities ... Einstein@Home now on S5 - like SETI@Home but LIGO data, download from http: ...
Photon astronomy sets indirect upper limits on GW - milestones for sensitivities ... Einstein@Home now on S5 - like SETI@Home but LIGO data, download from http: ...
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The Spin Periods of Millisecond X-Ray Pulsars and the Possible Role of Gravitational Radiation PowerPoint PPT Presentation
The Spin Periods of Millisecond X-Ray Pulsars and the Possible Role of Gravitational Radiation - For accreting pulsars, X-ray observations can measure spin by tracing rotating 'hot spots' ... Spreading hot spot on rotating NS surface yields 'nuclear-powered ...
For accreting pulsars, X-ray observations can measure spin by tracing rotating 'hot spots' ... Spreading hot spot on rotating NS surface yields 'nuclear-powered ...
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Deep Chandra Observations of LMXB Populations in Normal Elliptical Galaxies PowerPoint PPT Presentation
Deep Chandra Observations of LMXB Populations in Normal Elliptical Galaxies - Deep Chandra Observations of LMXB Populations in Normal Elliptical Galaxies
Deep Chandra Observations of LMXB Populations in Normal Elliptical Galaxies
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INPE%20Advanced%20Course%20on%20Compact%20Objects%20Course%20IV:%20Accretion%20Processes%20in%20Neutron%20Stars%20 PowerPoint PPT Presentation
INPE%20Advanced%20Course%20on%20Compact%20Objects%20Course%20IV:%20Accretion%20Processes%20in%20Neutron%20Stars%20 - 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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Gravitational Wave Astrophysics, Compact Binaries, and Numerical Relativity PowerPoint PPT Presentation
Gravitational Wave Astrophysics, Compact Binaries, and Numerical Relativity - Title: PowerPoint Presentation Author: Joan M. Centrella Last modified by: Joan Centrella Created Date: 9/7/2001 3:31:51 PM Document presentation format
Title: PowerPoint Presentation Author: Joan M. Centrella Last modified by: Joan Centrella Created Date: 9/7/2001 3:31:51 PM Document presentation format
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X-ray Binaries PowerPoint PPT Presentation
X-ray Binaries - Dipper iron line spectrum. Essentially every dipper shows evidence for highly ionized iron obsorption ... Dippers: Smale et al. 1988 MNRAS 232 647 ...
Dipper iron line spectrum. Essentially every dipper shows evidence for highly ionized iron obsorption ... Dippers: Smale et al. 1988 MNRAS 232 647 ...
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FROM SOFT TO HARD XRAY EMISSION PowerPoint PPT Presentation
FROM SOFT TO HARD XRAY EMISSION - B ~ 108 G. Rm (Falanga, Bonnet-Bidaud, Poutanen et al. 2005) ? ... Soft time lag: Downscattering of hard photons vs GR Doppler boosting ...
B ~ 108 G. Rm (Falanga, Bonnet-Bidaud, Poutanen et al. 2005) ? ... Soft time lag: Downscattering of hard photons vs GR Doppler boosting ...
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The X-ray source population studies in nearby galaxies PowerPoint PPT Presentation
The X-ray source population studies in nearby galaxies - The Xray source population studies in nearby galaxies
The Xray source population studies in nearby galaxies
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The states of Scorpius X-1 v.s. the 107 events PowerPoint PPT Presentation
The states of Scorpius X-1 v.s. the 107 events - Good Time Intervals ... Time before SAA or 30min after entering SAA ... (exposure: 15,168 sec) Take this data as an example: Observe time: Apr. 18~24, 1997 ...
Good Time Intervals ... Time before SAA or 30min after entering SAA ... (exposure: 15,168 sec) Take this data as an example: Observe time: Apr. 18~24, 1997 ...
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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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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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FOCUSING OPTICS WITH MOSAIC CRYSTALS PowerPoint PPT Presentation
FOCUSING OPTICS WITH MOSAIC CRYSTALS - Title: FOCUSING OPTICS WITH MOSAIC CRYSTALS Author: Your User Name Last modified by: filippo Document presentation format: Presentazione su schermo
Title: FOCUSING OPTICS WITH MOSAIC CRYSTALS Author: Your User Name Last modified by: filippo Document presentation format: Presentazione su schermo
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Neutron Stars PowerPoint PPT Presentation
Neutron Stars - Neutron Stars Neutron Stars Discovery of neutron (1932) Neutron Star (1934) Landau (unpublished) Baade & Zwicky With all reserve we advance the view that ...
Neutron Stars Neutron Stars Discovery of neutron (1932) Neutron Star (1934) Landau (unpublished) Baade & Zwicky With all reserve we advance the view that ...
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Cool discs, hot flows PowerPoint PPT Presentation
Cool discs, hot flows - Title: Presentazione di PowerPoint Author: Andrea Santangelo Last modified by: Tiziana Di Salvo Created Date: 6/29/2002 5:35:55 AM Document presentation format
Title: Presentazione di PowerPoint Author: Andrea Santangelo Last modified by: Tiziana Di Salvo Created Date: 6/29/2002 5:35:55 AM Document presentation format
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Kick velocity PowerPoint PPT Presentation
Kick velocity - Kick velocity Why do neutron stars move so rapidly? Stars vs. Neutron Stars Pulsar velocity distribution SN explosions should not be symmetric! SN and kick explosion ...
Kick velocity Why do neutron stars move so rapidly? Stars vs. Neutron Stars Pulsar velocity distribution SN explosions should not be symmetric! SN and kick explosion ...
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Pr PowerPoint PPT Presentation
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 Search For Gravitation Radiation From Periodic Sources PowerPoint PPT Presentation
The Search For Gravitation Radiation From Periodic Sources - Figures: K. S. Thorne gr-qc/9704042; Brady, Creighton, Cutler, Schutz gr-qc/9702050. ... Figure: Brady ITP seminar summer 2000. Amplitude Modulation. Figure: D. ...
Figures: K. S. Thorne gr-qc/9704042; Brady, Creighton, Cutler, Schutz gr-qc/9702050. ... Figure: Brady ITP seminar summer 2000. Amplitude Modulation. Figure: D. ...
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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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X-ray Studies of Millisecond Pulsars in Globular Clusters PowerPoint PPT Presentation
X-ray Studies of Millisecond Pulsars in Globular Clusters - Slavko Bogdanov, Craig Heinke, Maureen van den Berg, Fernando Camilo, Paulo Freire and ... (Grindlay, Portegies Zwart & McMillan 2006, Nature Physics, 2, 116) ...
Slavko Bogdanov, Craig Heinke, Maureen van den Berg, Fernando Camilo, Paulo Freire and ... (Grindlay, Portegies Zwart & McMillan 2006, Nature Physics, 2, 116) ...
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Accretion Power in Astrophysics PowerPoint PPT Presentation
Accretion Power in Astrophysics - If accretor has mass M and radius R, gravitational energy release/mass is ... Launching and collimation not understood probably requires. toroidal magnetic field ...
If accretor has mass M and radius R, gravitational energy release/mass is ... Launching and collimation not understood probably requires. toroidal magnetic field ...
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Results from Galactic Source Observations with VERITAS PowerPoint PPT Presentation
Results from Galactic Source Observations with VERITAS - ... ns.adobe.com/xap ... xmlns:tiff='http://ns.adobe.com/tiff/1.0/' tiff:Orientation ... xmlns:exif='http://ns.adobe.com/exif/1.0/' exif:PixelXDimension 792 ...
... ns.adobe.com/xap ... xmlns:tiff='http://ns.adobe.com/tiff/1.0/' tiff:Orientation ... xmlns:exif='http://ns.adobe.com/exif/1.0/' exif:PixelXDimension 792 ...
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Upper-limit on Sco X-1 S2 preliminary results PowerPoint PPT Presentation
Upper-limit on Sco X-1 S2 preliminary results - ... 5x10-22 - 3x10-21 depending on detector and frequency band (but only 2 frot) No analysis has been carried out on the band corresponding to 4/3 frot ...
... 5x10-22 - 3x10-21 depending on detector and frequency band (but only 2 frot) No analysis has been carried out on the band corresponding to 4/3 frot ...
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Gravitational wave astronomy PowerPoint PPT Presentation
Gravitational wave astronomy - Passing GW causes changes in the interferometer arm lengths. ... Of known pulsars Crab pulsar is most promising source, also possible pulsar in SN1987A remnant. ...
Passing GW causes changes in the interferometer arm lengths. ... Of known pulsars Crab pulsar is most promising source, also possible pulsar in SN1987A remnant. ...
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GRAVITATIONAL WAVES FROM PULSATIONS OF COMPACT STARS PowerPoint PPT Presentation
GRAVITATIONAL WAVES FROM PULSATIONS OF COMPACT STARS - Stergioulas N., 'Rotating Stars in Relativity', Living Reviews in Relativity, 6, ... In 2D Newtonian simulations a late-time (t 400ms) excitation of g-modes in ...
Stergioulas N., 'Rotating Stars in Relativity', Living Reviews in Relativity, 6, ... In 2D Newtonian simulations a late-time (t 400ms) excitation of g-modes in ...
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The Frequencies and Timescales Associated With Gravitational Wave Radiation From Compact Stars PowerPoint PPT Presentation
The Frequencies and Timescales Associated With Gravitational Wave Radiation From Compact Stars - Center for Gravitational Wave Phenomenology. Penn State University. 23 - 27 October 2002 ... Purely Hydrodynamical, in the presence of Newtonian gravity ...
Center for Gravitational Wave Phenomenology. Penn State University. 23 - 27 October 2002 ... Purely Hydrodynamical, in the presence of Newtonian gravity ...
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The slides in this collection are all related and should be useful in preparing a presentation on SI PowerPoint PPT Presentation
The slides in this collection are all related and should be useful in preparing a presentation on SI - Category 2: Transient in X-rays with Vquiescence brighter than 20 (8 targets) Category 3: Transient with Vquiescence fainter than 20 but Voutburst brighter than 20 ...
Category 2: Transient in X-rays with Vquiescence brighter than 20 (8 targets) Category 3: Transient with Vquiescence fainter than 20 but Voutburst brighter than 20 ...
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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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Neutron Stars PowerPoint PPT Presentation
Neutron Stars - For the Crab pulsar, P = 33 ms so the density must be greater than 1.3 1011 g cm ... The time that it takes for the pulsar to slow down is ...
For the Crab pulsar, P = 33 ms so the density must be greater than 1.3 1011 g cm ... The time that it takes for the pulsar to slow down is ...
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Neutron Star Observables, Masses, Radii and Magnetic Fields PowerPoint PPT Presentation
Neutron Star Observables, Masses, Radii and Magnetic Fields - Niels Bohr CompSchool Compact Objects Neutron Star Observables, Masses, Radii and Magnetic Fields Feryal Ozel University of Arizona Lecture 1: Surfaces of Neutron Stars
Niels Bohr CompSchool Compact Objects Neutron Star Observables, Masses, Radii and Magnetic Fields Feryal Ozel University of Arizona Lecture 1: Surfaces of Neutron Stars
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Key issues for hard X-ray emission from accreting black-hole and neutron-star sources PowerPoint PPT Presentation
Key issues for hard X-ray emission from accreting black-hole and neutron-star sources - Key issues for hard Xray emission from accreting blackhole and neutronstar sources
Key issues for hard Xray emission from accreting blackhole and neutronstar sources
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The Spin Periods of Millisecond X-Ray Pulsars and the Possible Role of Gravitational Radiation PowerPoint PPT Presentation
The Spin Periods of Millisecond X-Ray Pulsars and the Possible Role of Gravitational Radiation - Pulsars in. Low-Mass X-Ray Binaries. Deepto Chakrabarty ... Gravitational potential energy released as X-rays, ... (e.g. Ghosh & Lamb 1979; Lamb & Yu 2005) ...
Pulsars in. Low-Mass X-Ray Binaries. Deepto Chakrabarty ... Gravitational potential energy released as X-rays, ... (e.g. Ghosh & Lamb 1979; Lamb & Yu 2005) ...
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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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Robotic Telescopes and Telescope Networks PowerPoint PPT Presentation
Robotic Telescopes and Telescope Networks - Lower cost (fewer staff, no night work, less travel) ... Cheap to set up. Filter / calibration etc. problems. Sociological problems ...
Lower cost (fewer staff, no night work, less travel) ... Cheap to set up. Filter / calibration etc. problems. Sociological problems ...
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Debades%20Bandyopadhyay PowerPoint PPT Presentation
Debades%20Bandyopadhyay - There must exist a critical angular velocity c above which the perturbation will ... Bulk viscosity coefficient due to modified Urca process of nucleons: ...
There must exist a critical angular velocity c above which the perturbation will ... Bulk viscosity coefficient due to modified Urca process of nucleons: ...
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Gravitational wave astronomy: observing the fabric of spacetime PowerPoint PPT Presentation
Gravitational wave astronomy: observing the fabric of spacetime - Gravitational wave astronomy: observing the fabric of spacetime
Gravitational wave astronomy: observing the fabric of spacetime
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a brief history of PowerPoint PPT Presentation
a brief history of - a brief history of andreas m ller theory group max camenzind lsw heidelberg http://www.lsw.uni-heidelberg.de/users/amueller student seminar mpia & lsw
a brief history of andreas m ller theory group max camenzind lsw heidelberg http://www.lsw.uni-heidelberg.de/users/amueller student seminar mpia & lsw
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INSTABILITIES OF ROTATING RELATIVISTIC STARS PowerPoint PPT Presentation
INSTABILITIES OF ROTATING RELATIVISTIC STARS - Watts, Andersson Rezzolla,Lamb,Markovic, Arras, Flanagan, Morsink, Shapiro ... Spruit Rezzola, Lamb, Shapiro. Levin, Ushomirsky R, Markovic, L, S ...
Watts, Andersson Rezzolla,Lamb,Markovic, Arras, Flanagan, Morsink, Shapiro ... Spruit Rezzola, Lamb, Shapiro. Levin, Ushomirsky R, Markovic, L, S ...
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Jean%20Cottam PowerPoint PPT Presentation
Jean%20Cottam - Jean Cottam
Jean Cottam
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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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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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