XIV Advanced School on Astrophysics Topic III: Observations of the Accretion Disks of Black Holes and Neutron Stars III.3: Accretion Disks of Non-Magnetic Neutron Stars
Discuss current developments (both here and elsewhere DESPEC, ... Points Cyril Varignon these LPC Caen (1999) 11/30/09. 10. Improvement with JENDL data set ...
Evolution of isolated neutron stars: young coolers and old accretors Sergei Popov (SAI) Plan of the talk Magnetic rotator Evolution of neutron stars: rotation ...
UCN are neutrons that are moving so slowly that they are ... How to generate matter-antimatter asymmetry? Belief: this is an effective theory below 100 GeV ...
INPE Advanced Course on Compact Objects Course IV: Accretion Processes in Neutron Stars & Black Holes Ron Remillard Kavli Center for Astrophysics and Space Research
Other techniques use a full least-squares fit to the pulse shape, eg. ... Least square fitting of scintillator pulses ... complex iterative fitting procedure is ...
... readings and a melt-rupture disk in the side-wall of the beam guide tube. ... A very rough conceptual design for a 1000 MWe plant has been developed. ...
Comparison between neutron data from HEND and gamma-ray data from GRS ... Take GRS spectra of surface of Mars for pixels 10x10 degree for time period: ...
PSR J1629-6902. 3 nearby Fermi-LAT sources. closest 5.1 away. 10. Data on Sample of Pulsars ... point for Hannestad-Raffelt function (n=3) was specified for PSR. ...
London, 27 Apr 2006. 1. Constraints on Neutron Star Cooling using Chandra ... EGRET. Pulsations observed with ROSAT and EGRET with periods matching the radio solution ...
Nuclear densities et excitations of exotic nuclei via direct reactions ACTIVITIES AND PERSPECTIVES Structure studies at the drip-lines : exemples, + exp-theory
... determinations and a linear least square fit using the 68% formal errors in ... Adding these to the linear square fit gives P0 = 8.39107 0.00005 s, dP/dt ...