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Interstellar Scintillation of the Double Pulsar J0737-3039: Effects of Anisotropy PowerPoint PPT Presentation
Interstellar Scintillation of the Double Pulsar J0737-3039: Effects of Anisotropy - Interstellar Scintillation of the Double Pulsar J0737-3039: Effects of Anisotropy ... pioneering analysis of the orbital modulation of millisecond binary PSR J1141-65. ...
Interstellar Scintillation of the Double Pulsar J0737-3039: Effects of Anisotropy ... pioneering analysis of the orbital modulation of millisecond binary PSR J1141-65. ...
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Neutron Star masses and radii PowerPoint PPT Presentation
Neutron Star masses and radii - ... Relativistic corrections and measurable parameters Shapiro delay Mass measurements Double pulsar J0737-3039 Masses for PSR J0737-3039 The most extreme ...
... Relativistic corrections and measurable parameters Shapiro delay Mass measurements Double pulsar J0737-3039 Masses for PSR J0737-3039 The most extreme ...
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LIGHT PSEUDOSCALAR BOSONS, PVLAS AND DOUBLE PULSAR J07373039 PowerPoint PPT Presentation
LIGHT PSEUDOSCALAR BOSONS, PVLAS AND DOUBLE PULSAR J07373039 - LIGHT PSEUDOSCALAR BOSONS, PVLAS AND DOUBLE PULSAR J0737-3039 ... Sic stantibus rebus.... INDEPENDENT CHECKS of PVLAS claim are COMPELLING! ...
LIGHT PSEUDOSCALAR BOSONS, PVLAS AND DOUBLE PULSAR J0737-3039 ... Sic stantibus rebus.... INDEPENDENT CHECKS of PVLAS claim are COMPELLING! ...
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A New Relativistic Binary Pulsar: Gravitational Wave Detection and Neutron Star Formation PowerPoint PPT Presentation
A New Relativistic Binary Pulsar: Gravitational Wave Detection and Neutron Star Formation - Gravitational Waves and Double Neutron Stars. Meet PSR J0737-3039: ... (Demorest et al. 2004) What will we learn in the near future ? ...
Gravitational Waves and Double Neutron Stars. Meet PSR J0737-3039: ... (Demorest et al. 2004) What will we learn in the near future ? ...
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Lecture1. Structure of Neutron Stars PowerPoint PPT Presentation
Lecture1. Structure of Neutron Stars - (see discussion in Nature). (Trumper) (Trumper) Massive NS: 2.1+/-0.3 solar masses (Trumper) PSR J0737-3039 (see Lattimer, Schutz astro-ph/0411470) ...
(see discussion in Nature). (Trumper) (Trumper) Massive NS: 2.1+/-0.3 solar masses (Trumper) PSR J0737-3039 (see Lattimer, Schutz astro-ph/0411470) ...
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Pulsar Timing with the GBT PowerPoint PPT Presentation
Pulsar Timing with the GBT - Are many of the fastest-spinning pulsars hidden? 5 of the 10 fastest-spinning pulsars show eclipses. ... Spin Freq. (Hz) Pulsar. Name. Are the frequencies ...
Are many of the fastest-spinning pulsars hidden? 5 of the 10 fastest-spinning pulsars show eclipses. ... Spin Freq. (Hz) Pulsar. Name. Are the frequencies ...
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Estimation of the Binary Pulsar Coalescence Rates, and the Detection Rates for Gravitational Wave De PowerPoint PPT Presentation
Estimation of the Binary Pulsar Coalescence Rates, and the Detection Rates for Gravitational Wave De - (e.g. LIGO, VIRGO, GEO600, TAMA300) Galactic merger rate. of DNS systems. Event rate estimation ... adapt the pulsar properties & orbital characteristics ...
(e.g. LIGO, VIRGO, GEO600, TAMA300) Galactic merger rate. of DNS systems. Event rate estimation ... adapt the pulsar properties & orbital characteristics ...
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Radio%20Astronomy PowerPoint PPT Presentation
Radio%20Astronomy - Radio Astronomy
Radio Astronomy
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Galactic Merger Rate of DNS Systems and Prospects for Detecting Gravitational Waves Chunglee Kim Nor PowerPoint PPT Presentation
Galactic Merger Rate of DNS Systems and Prospects for Detecting Gravitational Waves Chunglee Kim Nor - Chunglee Kim (Northwestern) with. Vicky Kalogera (NU), Duncan R. Lorimer (Manchester) ... Method - Modeling & Simulation (Kim et al. 2003, ApJ, 584, 985 ) ...
Chunglee Kim (Northwestern) with. Vicky Kalogera (NU), Duncan R. Lorimer (Manchester) ... Method - Modeling & Simulation (Kim et al. 2003, ApJ, 584, 985 ) ...
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Chapter 13: The Deaths of Stars PowerPoint PPT Presentation
Chapter 13: The Deaths of Stars - Chapter 13: The Deaths of Stars The Helix Nebula Planetary Nebulae From Supergiants to White Dwarfs Structure of an Old Low-Mass Star Structure of an Old High-Mass ...
Chapter 13: The Deaths of Stars The Helix Nebula Planetary Nebulae From Supergiants to White Dwarfs Structure of an Old Low-Mass Star Structure of an Old High-Mass ...
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Radio Pulsars PowerPoint PPT Presentation
Radio Pulsars - Longitude of periastron 226.57528(6) degrees. Time of periastron 46443.99588319(3) (MJD) ... Survey region: 220o gl 260o, -60o gb 60o ...
Longitude of periastron 226.57528(6) degrees. Time of periastron 46443.99588319(3) (MJD) ... Survey region: 220o gl 260o, -60o gb 60o ...
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Radio Astronomy and the NRAO PowerPoint PPT Presentation
Radio Astronomy and the NRAO - Radio Astronomy
Radio Astronomy
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Ignazio Bombaci Dipartimento di Fisica PowerPoint PPT Presentation
Ignazio Bombaci Dipartimento di Fisica - Achievements and Perspectives in Low-Energy QCD with strangeness ...
Achievements and Perspectives in Low-Energy QCD with strangeness ...
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Revised Inspiral Rates for Double Neutron Star Systems Chunglee Kim Northwestern PowerPoint PPT Presentation
Revised Inspiral Rates for Double Neutron Star Systems Chunglee Kim Northwestern - 5 systems are known in our Galaxy. 2 coalescing systems in the Galactic disk. ... populate a model galaxy with Ntot PSRs (same Ps & Porb) Nobs follows the ...
5 systems are known in our Galaxy. 2 coalescing systems in the Galactic disk. ... populate a model galaxy with Ntot PSRs (same Ps & Porb) Nobs follows the ...
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Binary population synthesis implications for gravitational wave sources PowerPoint PPT Presentation
Binary population synthesis implications for gravitational wave sources - Are the methods credible? Binary compact objects. Only few ... AURIGA, EXPLORER, NAUTILUS. First detection attempts. J. Weber the 1960-ies. Sensitivity ...
Are the methods credible? Binary compact objects. Only few ... AURIGA, EXPLORER, NAUTILUS. First detection attempts. J. Weber the 1960-ies. Sensitivity ...
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GWDAW - Annecy PowerPoint PPT Presentation
GWDAW - Annecy - Searching for gravitational waves from known pulsars Matthew Pitkin for the LIGO Scientific Collaboration Summary of work to date There have been three science runs ...
Searching for gravitational waves from known pulsars Matthew Pitkin for the LIGO Scientific Collaboration Summary of work to date There have been three science runs ...
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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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Michael Kramer PowerPoint PPT Presentation
Michael Kramer - Michael Kramer
Michael Kramer
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An FX software correlator for VLBI PowerPoint PPT Presentation
An FX software correlator for VLBI - Averaging the product of signals at two telescopes gives visibility ... FPGA used for unpacking/fringe rotating and FFT. Possibly incorporate cross-multiply ...
Averaging the product of signals at two telescopes gives visibility ... FPGA used for unpacking/fringe rotating and FFT. Possibly incorporate cross-multiply ...
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How to test the Einstein gravity using gravitational waves PowerPoint PPT Presentation
How to test the Einstein gravity using gravitational waves - How to test the Einstein gravity using gravitational waves Gravitational waves Takahiro Tanaka (YITP, Kyoto university) Based on the work in collaboration with
How to test the Einstein gravity using gravitational waves Gravitational waves Takahiro Tanaka (YITP, Kyoto university) Based on the work in collaboration with
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THEORETICAL ASPECTS PowerPoint PPT Presentation
THEORETICAL ASPECTS - Consider a photon beam in vacuo with k along the z-axis. ... 'Sic stantibus rebus'.... INDEPENDENT CHECKS of PVLAS claim look COMPELLING. ...
Consider a photon beam in vacuo with k along the z-axis. ... 'Sic stantibus rebus'.... INDEPENDENT CHECKS of PVLAS claim look COMPELLING. ...
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Chapter 13: The Deaths of Stars PowerPoint PPT Presentation
Chapter 13: The Deaths of Stars - Where do heavy elements on the Earth like carbon, silicon, oxygen, iron, and ... Sirius and White Dwarf. Sirius B, a white dwarf, at the five o'clock position ...
Where do heavy elements on the Earth like carbon, silicon, oxygen, iron, and ... Sirius and White Dwarf. Sirius B, a white dwarf, at the five o'clock position ...
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Scuola nazionale de Astrofisica PowerPoint PPT Presentation
Scuola nazionale de Astrofisica - Galactic distribution of pulsars. Birth rate and evolution ... First searches used chart recorders and detected individual pulses ...
Galactic distribution of pulsars. Birth rate and evolution ... First searches used chart recorders and detected individual pulses ...
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Pulsars, Gravitational Waves PowerPoint PPT Presentation
Pulsars, Gravitational Waves - Galaxy formation. Binary black holes in galaxies. Neutron-star formation in supernovae ... in gravitational field of the Galaxy (Weisberg & Taylor 2005) ...
Galaxy formation. Binary black holes in galaxies. Neutron-star formation in supernovae ... in gravitational field of the Galaxy (Weisberg & Taylor 2005) ...
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Gravitational waves and fundamental physics PowerPoint PPT Presentation
Gravitational waves and fundamental physics - Gravitational waves and. fundamental physics. Michele Maggiore. Universit ... What can we hope to learn about fundamental physics. from the observation of GWs ...
Gravitational waves and. fundamental physics. Michele Maggiore. Universit ... What can we hope to learn about fundamental physics. from the observation of GWs ...
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New Views of Compact Object Mergers Via Short Gamma-Ray Bursts PowerPoint PPT Presentation
New Views of Compact Object Mergers Via Short Gamma-Ray Bursts - New Views of Compact Object Mergers Via Short Gamma-Ray Bursts ... J. Wren, LANL. B. L. Lee, U. Toronto. P. J. McCarthy, Carnegie. D. C. Murphy, Carnegie ...
New Views of Compact Object Mergers Via Short Gamma-Ray Bursts ... J. Wren, LANL. B. L. Lee, U. Toronto. P. J. McCarthy, Carnegie. D. C. Murphy, Carnegie ...
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Neutron star masses: dwarfs, giants and neighbors PowerPoint PPT Presentation
Neutron star masses: dwarfs, giants and neighbors - Neighbors: young and slim. Initial NS mass spectrum is unknown ... Young close-by NSs are slim 1.4Msun. Mass constraint can be useful for ...
Neighbors: young and slim. Initial NS mass spectrum is unknown ... Young close-by NSs are slim 1.4Msun. Mass constraint can be useful for ...
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Solar vicinity, close-by young isolated NSs, and tests of cooling curves PowerPoint PPT Presentation
Solar vicinity, close-by young isolated NSs, and tests of cooling curves - Solar vicinity, close-by young isolated NSs, and tests of cooling curves Sergei Popov (Sternberg Astronomical Institute) Co-authors: H.Grigorian, R. Turolla, D. Blaschke
Solar vicinity, close-by young isolated NSs, and tests of cooling curves Sergei Popov (Sternberg Astronomical Institute) Co-authors: H.Grigorian, R. Turolla, D. Blaschke
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Pulsares PowerPoint PPT Presentation
Pulsares - High mean orbital velocities and accelerations than other binary ... Allow for tests of General Relativity and alternate theories ... Neutron-star masses ...
High mean orbital velocities and accelerations than other binary ... Allow for tests of General Relativity and alternate theories ... Neutron-star masses ...
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Aperture Photometry and Time Series Analysis of Selected Blazars PowerPoint PPT Presentation
Aperture Photometry and Time Series Analysis of Selected Blazars - ... of the signal, to determine auto/cross-correlations and time lags, transient ... Intra-day (hours) variations can be detected for the brightest gamma-ray blazars. ...
... of the signal, to determine auto/cross-correlations and time lags, transient ... Intra-day (hours) variations can be detected for the brightest gamma-ray blazars. ...
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Expected Coalescence Rate of NSNS Binaries for Ground Based Interferometers PowerPoint PPT Presentation
Expected Coalescence Rate of NSNS Binaries for Ground Based Interferometers - spiral (fS=65%) and elliptical (fE=35%) galaxies. same fb and bNS as for the Milky Way ... elliptical galaxy star formation efficiency and IMF estimated from ...
spiral (fS=65%) and elliptical (fE=35%) galaxies. same fb and bNS as for the Milky Way ... elliptical galaxy star formation efficiency and IMF estimated from ...
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Scuola%20nazionale%20de%20Astrofisica PowerPoint PPT Presentation
Scuola%20nazionale%20de%20Astrofisica - Lorimer & Kramer 2005 'Handbook of Pulsar Astronomy' Books. Review Articles ... Lorimer 2005: Binary and MS pulsars. Will, 2006: GR theory and experiment ...
Lorimer & Kramer 2005 'Handbook of Pulsar Astronomy' Books. Review Articles ... Lorimer 2005: Binary and MS pulsars. Will, 2006: GR theory and experiment ...
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DIRECT DETECTION OF STRONG GALAXYGALAXY LENSING IN SDSS : usage of photometry catalogs PowerPoint PPT Presentation
DIRECT DETECTION OF STRONG GALAXYGALAXY LENSING IN SDSS : usage of photometry catalogs - High-resolution IR and optical data. Strongly lensed galaxies in SDSS ... Forming multiple images of arc and knots. Red galaxy SED at low-z. Different SED at high-z ...
High-resolution IR and optical data. Strongly lensed galaxies in SDSS ... Forming multiple images of arc and knots. Red galaxy SED at low-z. Different SED at high-z ...
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Theory Summary H' Stcker, FIAS PowerPoint PPT Presentation
Theory Summary H' Stcker, FIAS - Theory Summary H' Stcker, FIAS
Theory Summary H' Stcker, FIAS
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Current and Future Science with NRAO Instruments PowerPoint PPT Presentation
Current and Future Science with NRAO Instruments - Cosmic geometry: Megamasers and a 3% measure of Ho ... Ho = 64 ( /-7) Already at HST Key project accuracy with 1 source! 14. HST ...
Cosmic geometry: Megamasers and a 3% measure of Ho ... Ho = 64 ( /-7) Already at HST Key project accuracy with 1 source! 14. HST ...
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The search for gravitational waves: physical motivations and experimental perspectives PowerPoint PPT Presentation
The search for gravitational waves: physical motivations and experimental perspectives - CHIPP meeting, Lausanne, 12/04/06. Why GW physics is interesting ... ALLEGRO (Louisiana), AURIGA (Padua), NAUTILUS(Rome) , EXPLORER (Cern) MiniGRAIL(Leiden) ...
CHIPP meeting, Lausanne, 12/04/06. Why GW physics is interesting ... ALLEGRO (Louisiana), AURIGA (Padua), NAUTILUS(Rome) , EXPLORER (Cern) MiniGRAIL(Leiden) ...
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Radio Pulsars and Gravity Studies Jim Cordes Cornell PowerPoint PPT Presentation
Radio Pulsars and Gravity Studies Jim Cordes Cornell - Radio Pulsars and Gravity Studies Jim Cordes Cornell
Radio Pulsars and Gravity Studies Jim Cordes Cornell
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Solar vicinity, closeby young isolated NSs, and tests of cooling curves PowerPoint PPT Presentation
Solar vicinity, closeby young isolated NSs, and tests of cooling curves - Later on: six brothers. RX J1856.5-3754. 5. Magnificent Seven. 9.44 ... in the low-frequency band (60-110 MHz) with the radio telescope in Pushchino. (back) ...
Later on: six brothers. RX J1856.5-3754. 5. Magnificent Seven. 9.44 ... in the low-frequency band (60-110 MHz) with the radio telescope in Pushchino. (back) ...
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Sources of gravitational waves for groundbased detectors PowerPoint PPT Presentation
Sources of gravitational waves for groundbased detectors - Free precession. Was thought to damp in 1yr (vortex pinning) ... 22, 1825 (2005): Observations say precession lasts 10yr, visible to galactic ...
Free precession. Was thought to damp in 1yr (vortex pinning) ... 22, 1825 (2005): Observations say precession lasts 10yr, visible to galactic ...
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Diversity across the P P Diagram PowerPoint PPT Presentation
Diversity across the P P Diagram - Two highly eccentric systems: 0.43 (I) and 0.35 (J) X-ray IDs in 47 Tuc ... Second SN doesn't disrupt the system but does make it eccentric ...
Two highly eccentric systems: 0.43 (I) and 0.35 (J) X-ray IDs in 47 Tuc ... Second SN doesn't disrupt the system but does make it eccentric ...
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Future Radio Synoptic Surveys PowerPoint PPT Presentation
Future Radio Synoptic Surveys - Future Radio Synoptic Surveys
Future Radio Synoptic Surveys
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Pulsares PowerPoint PPT Presentation
Pulsares - Los pulsares son estrellas de neutrones en rotaci n. ... interstellar medium causes lower radio frequencies to arrive at the Earth with ...
Los pulsares son estrellas de neutrones en rotaci n. ... interstellar medium causes lower radio frequencies to arrive at the Earth with ...
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