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: ...
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 ...
High mean orbital velocities and accelerations than other binary ... Allow for tests of General Relativity and alternate theories ... Neutron-star masses ...
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. ...
... 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 ...
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 ...
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 ...
Observational Perspective. Simon Johnston. Australia Telescope National Facility. CSIRO ... A whole zoo of new and interesting objects. Magnetars. AXPs / SGRs ...
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 ...
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 ...
Slavko Bogdanov, Craig Heinke, Maureen van den Berg, Fernando Camilo, Paulo Freire and ... (Grindlay, Portegies Zwart & McMillan 2006, Nature Physics, 2, 116) ...
Importance of Compton scattering on X-ray spectra of Millisecond Pulsars and ... Method of WD mass estimations. Shock wave standing above WD surface ...
The current theoretical model states that a pulsar is a highly magnetized, ... Retardation, aberration and the geometry of the magnetic field lines predict ...
(2) Gamma-ray studies cannot find any differences. between radio-loud and radio-quiet pulsars ... Only one target lacks obvious counterpart... Nearby source is ...
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' ...
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 ...
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 ...
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 ...
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 ...
broad (zero-centred L) noise for low and high frequencies. peaked noise for intermediate frequencies. HMXB vs LMXB: differences. different topology ...