Glitches; the Link Between the Typical Radio Pulsars and the Anomalous X-ray Pulsars ... Theoretical models for pulsar glitches; star quake and vortex creep ...
Pulsars - isolated neutron stars - radiate energy via slowing ... Brightening on boundaries between closed and open lines may produce subpulses. Light Cylinder ...
Workshop pulsars 16-17 Janvier 2006. Pulsars et chelles de temps. G rard Petit ... D. R. Lorimer, 'Binary and Millisecond Pulsars at the New Millennium', http: ...
High mean orbital velocities and accelerations than other binary ... Allow for tests of General Relativity and alternate theories ... Neutron-star masses ...
Known radio pulsars appear to emit short pulses of radio radiation with pulse ... ( From the Handbook of Pulsar Astronomy, by Lorimer and Kramer) 46. Pulsar population ...
You are listening to a radio recording of a pulsar (the Vela pulsar) of mass ... parameters have been obtained; precession due to relativistic spin-orbit ...
... densities, exotica such as strangeness-bearing baryons, condensed mesons (pion ... up, down, and strange quarks (the charm, bottom, and top quarks are too massive ...
Neutron stars are the collapsed cores of massive stars, ~15 to 30 times the mass ... but deeper down the pressure is high enough that the atomic weights rise ...
OUTLINE (What is a new in hard X-rays) I. Hard X-ray spectra of X-ray pulsars ... Timing analysis of the INTEGRAL/IBIS data of X-ray pulsars. in narrow energy bands. ...
GALACTIC ASTRONOMY (II): PULSARS. Jon Marcaide. ASI, Castel San Pietro Terme, 18 September 2001 ... on models of Galactic electron density distribution obtained ...
Galaxy formation. Binary black holes in galaxies. Neutron-star formation in supernovae ... in gravitational field of the Galaxy (Weisberg & Taylor 2005) ...
X-Ray Pulsars: Accretion and Variability. These talks will occur weekly ... Akshay Kulkarni. Cornell University. Wednesday August 3 @ 3pm in SS 301 ...
Simulated the gravity wave spectrum for gravity wave backgrounds. 15th April, 2004 ... Earth and a pulsar as two free masses and monitoring their apparent motion by ...
Effet Doppler d au mouvement orbital autour du Soleil et la rotation de la Terre: ... signal: sinuso de amortie. filtre adapt 2 param tres: masse et ...
... usually in binary. systems with O-B spectral class massive stars. ... Required new generation of X-ray telescopes and observatories: NeXT, Spectrum-XG, XEUS ...
Developed and applied to data of SAS-2, COS-B, and EGRET. The ... Assume a stretch of data that is 1 week long: tobs = 6x105 sec. f1=0.2 Hz to f2=1000 Hz : ...
Amount of gravitational radiation emitted from a binary star ... Fast Chirp Transform and Fresnel Integrals. Intrinsic frequency modes for pulsar rotation: ...
Observational Perspective. Simon Johnston. Australia Telescope National Facility. CSIRO ... A whole zoo of new and interesting objects. Magnetars. AXPs / SGRs ...
They are created in a supernova explosion near the end of a ... Textbook: Horizons: Exploring the Universe by Michael A. Seeds. Lecture Notes: Dr. M. Richards ...
Investigating Pulsars with DC2 and GLAST Data. Review of possible DC2 source classes ... Suggestions for investigation. Alice K. Harding (NASA Goddard) Possible ...
Accretion always considered a viable mechanism to sustain GW emission ... Ephemeris. Phase of Sco X-1 on the orbit at a given epoch 'Loop' over bandwidth ...
Fix the problem with visualization of ellipticity of known pulsar. ... Ellipticity for Pulsar Emitting. at 500 Hz 1Kpc distance I y IT. Histogram for Crab Data ...
The current theoretical model states that a pulsar is a highly magnetized, ... Retardation, aberration and the geometry of the magnetic field lines predict ...
Slavko Bogdanov, Craig Heinke, Maureen van den Berg, Fernando Camilo, Paulo Freire and ... (Grindlay, Portegies Zwart & McMillan 2006, Nature Physics, 2, 116) ...
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 ...
Geodetic Precession. So far: General Relativity has passed. all tests with ... Visible as a precession of the orbit: Measure higher order derivatives of secular ...
loud and radio-quiet, gamma-ray pulsars from the Galaxy and the Gould Belt' ... 'Galactic Populations of Radio and Gamma-Ray Pulsars in the Polar Cap Model' ...
Importance of Compton scattering on X-ray spectra of Millisecond Pulsars and ... Method of WD mass estimations. Shock wave standing above WD surface ...
(2) Gamma-ray studies cannot find any differences. between radio-loud and radio-quiet pulsars ... Only one target lacks obvious counterpart... Nearby source is ...
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 ...
Scripts allow to perform the basic data reduction in automatic way (applying ... Scripts can be done using bash/tcsh shell or using scripting languages like Python ...
Only a very modest reduction in calculation for a given f-dot, since the ... For each photon, calculate the differences between its time-of-arrival and those ...
For accreting pulsars, X-ray observations can measure spin by tracing rotating 'hot spots' ... Spreading hot spot on rotating NS surface yields 'nuclear-powered ...
Radio beam geometry and velocity kick distribution Arzoumanian, Chernoff & Cordes (2002) ... to 978 radio pulsars (Galactic plane) to 120 supernovae in the Gould Belt ...
mission tr s haute nergie des pl rions. M canismes d'acc l ration et rayons cosmiques ... Vent du pulsar vers le milieu ambient issu des calottes polaires ...
... to bursts... 150 seconds,no relation with bursts. Many many many non-pulsating sources... No special characteristic: no burst, no extreme behavior, no energy ...