'Millisecond pulsars' presentation slideshows

Last Section of AY4

Last Section of AY4. Last quiz, Thursday, March 13 Optional Final on March 17, 12-3pm Neutron stars, pulsars, x-ray binaries Relativity Black Holes The Big Bang and cosmology. Neutron Stars. There is a last test of SNII theory

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Pulsar Astronomy and Astrophysics Frontiers

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Pulsar Searching and Timing

Pulsar Searching and Timing. - with a pplication to FAST. R. N. Manchester. CSIRO Astronomy and Space Science Sydney Australia. Summary. I ntroduction to pulsars and timing Binary pulsar timing Pulsar timing arrays Searching for pulsars Prospects for FAST.

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Fundamental Physics and Astrophysics using Pulsars and the SKA

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ASTR 1102-002 2008 Fall Semester

ASTR 1102-002 2008 Fall Semester. Joel E. Tohline, Alumni Professor Office: 247 Nicholson Hall [Slides from Lecture17]. Interacting Binary Stars. Interacting Binary Stars. Definition: A binary is said to be interacting if mass is transferred or exchanged between the components. Note:

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Les Pulsars gamma avec GLAST

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The Search for Gravitational Waves using Pulsar Timing

The Search for Gravitational Waves using Pulsar Timing. R. N. Manchester. CSIRO Astronomy and Space Science Sydney Australia. Summary. Brief introduction to pulsars and timing Detection of GW using pulsar timing Pulsar Timing Array (PTA) projects Current status and future prospects.

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Accretion-Powered Millisecond Pulsars Juri Poutanen (University of Oulu, Finland) Plan:

Accretion-Powered Millisecond Pulsars Juri Poutanen (University of Oulu, Finland) Plan: X-ray bursts oscillations Millisecond pulsars SAX J1808.4-3658: pulse-resolved spectra, energy-dependent pulse profiles (1998, 2002 outbursts) XTE J1751-305 XTE J1807-294 Model and results

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One antenna on each side of spacecraft, to see whole sky, i.e., as many GPS satellites at

(Two of these on spacecraft.). Serial communications. One of the two redundant antennae. Power. One antenna on each side of spacecraft, to see whole sky, i.e., as many GPS satellites at a time as possible. Receiver handles them both together. Absolute timestamp end-to-end test.

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Detection of Gravitational Waves with Pulsar Timing

Detection of Gravitational Waves with Pulsar Timing. R. N. Manchester. Australia Telescope National Facility, CSIRO Sydney Australia. Summary. Brief review of pulsar properties and timing Detection of gravitational waves Pulsar Timing Array (PTA) projects

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R. N. Manchester

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Present and future of pulsar research: the Italian contribute

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Neutron Star Zoo: radio pulsars, magnetars , RRATs, CCOs, and more

Neutron Star Zoo: radio pulsars, magnetars , RRATs, CCOs, and more. Stephen C.-Y. Ng McGill University. Special thanks to Vicky Kaspi for some materials in this talk. Overview. Since the first pulsar discovered 40 yrs ago, they are all thought to be: b orn spinning fast in SNRs

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Neutron Stars 4: Magnetism

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Neutron Stars 2: Phenomenology

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Parsec-scale Constraints on the ISM From the Millisecond Pulsars in Terzan5

Jason Hessels (McGill) Ingrid Stairs (UBC) David Kaplan (MIT). Fernando Camilo (Columbia) Paulo Freire (Arecibo Obs) Victoria Kaspi (McGill). Parsec-scale Constraints on the ISM From the Millisecond Pulsars in Terzan5. Scott Ransom (NRAO Charlottesville).

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Searches for Young Pulsars

Searches for Young Pulsars. Tania Regimbau OCA/Nice. Triaxial Emission. Gravitational Wave polarization amplitudes from a triaxial rotating NS:. The ideal pulsar is fast , close , with large equatorial deformation !.

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He star evolutionary channel to intermediate-mass binary pulsars with a short-orbital-period

He star evolutionary channel to intermediate-mass binary pulsars with a short-orbital-period. Chen Wen-Cong. School of Physics, Peking University Department of Physics, Shangqiu Normal University. Normal Radio Pulsars and Millisecond pulsars. Normal radio pulsars. MSPs.

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Radio Observations of X-ray Binaries : Solitary and Binary Millisecond Pulsars

Radio Observations of X-ray Binaries : Solitary and Binary Millisecond Pulsars. Jeong-Sook Kim 1 & Soon-Wook Kim 2 Department of Space Science and Astronomy in KyungHee University Korea Astronomy and Space Science Institute. Abstract.

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