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 ...
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 ...
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
For accreting pulsars, X-ray observations can measure spin by tracing rotating 'hot spots' ... Spreading hot spot on rotating NS surface yields 'nuclear-powered ...
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 ...
Probing the neutron star physics with accreting neutron stars (part 2) ... Use of three wonderful satellites: Chandra, XMM-Newton, RXTE. Outburst vs. quiescence ...
Analysing X-ray spectra from Beppo SAX authors found that strong wind from WR ... Type I bursts are observed in systems with highly eccentric orbits. ...
INPE Advanced Course on Compact Objects Course IV: Accretion Processes in Neutron Stars & Black Holes Ron Remillard Kavli Center for Astrophysics and Space Research
Mass & Radius of Compact Objects Fastest pulsar and its stellar EOS CHENGMIN ZHANG National Astronomical Observatories Chinese Academy of Sciences, Beijing
... densities, exotica such as strangeness-bearing baryons, condensed mesons (pion ... up, down, and strange quarks (the charm, bottom, and top quarks are too massive ...
Different Manifestations of Neutron Stars Isolated (Magnetic) Neutron Stars: From Interior to surface to magnetosphere Accreting Neutron Stars Merging Neutron Stars
Determining the Equation of State of Ultradense Matter with the Advanced X-ray Timing Array (AXTAR) Deepto Chakrabarty (MIT) Paul S. Ray (NRL) Tod Strohmayer (NASA/GSFC)
Slavko Bogdanov, Craig Heinke, Maureen van den Berg, Fernando Camilo, Paulo Freire and ... (Grindlay, Portegies Zwart & McMillan 2006, Nature Physics, 2, 116) ...
Where: ~ 2.6 outburst mass transfer rate in unit of 10-10 M?/yr ... mechanism responsible for the switch from the outburst. to the quiescent phases (and vice versa) ...
(Towards) A unified model of X-ray variability in X-ray binaries and AGN. Phil ... L(t) has a Gaussian distribution, so X(t) has a lognormal distribution...
Eclipses (10s min days) Accretion disks (~ms years) Transients (X-ray novae) ... Distributed as 2 with 2 degrees of freedom (d.o.f.) for the Leahy normalization ...
... to bursts... 150 seconds,no relation with bursts. Many many many non-pulsating sources... No special characteristic: no burst, no extreme behavior, no energy ...