Studies of thermonuclear X-ray bursts can be very useful to constrain the spin rate, mass and radius of a neutron star approaching EOS model of high density cold matter in the neutron star cores. +k Extensive observation and analysis of the data from the rising portions of the bursts - modeling of burst oscillations and thermonuclear flame spreading. +k Theoretical study of thermonuclear flame spreading on the rapidly spinning neutron stars should be done considering all the main physical effects (including magnetic field, nuclear energy generation, Coriolis effect, strong gravity, etc.)
Analysis of observations of the X-ray emission produced by accreting neutron stars with millisecond ...
© 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society....
Neutron stars, with their strong surface gravity, have interestingly short timescales for the sedime...
This viewgraph presentation describes neutron stars and thermonuclear x ray bursts. The contents inc...
Observations of Type I X-ray bursts have long been taken as evidence that the sources are neutron st...
Observations of thermonuclear (Type I) X-ray bursts from neutron stars in low mass X-ray binaries (L...
Since the advent of powerful new X-ray observatories, NASA's Rossi X-ray Timing Explorer (RXTE), the...
Neutron stars are the most compact stars that can be directly observed, which makes them ideal labor...
Neutron stars offer a unique environment in which to develop and test theories of the strong force. ...
Results of various observations of common type I X-ray bursts are discussed with respect to the theo...
I review our understanding of the thermonuclear instabilities on accreting neutron stars that produc...
Burst oscillations, a phenomenon observed in a significant fraction of Type I (thermonuclear) X-ray ...
Observational evidence has been accumulating that thermonuclear X-ray bursts ignited on the surface ...
Unstable thermonuclear burning on the surface of accreting neutron stars is commonly observed as t...
Neutron stars (NS) are the most compact objects that can be directly observed. They can be used to s...
Analysis of observations of the X-ray emission produced by accreting neutron stars with millisecond ...
© 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society....
Neutron stars, with their strong surface gravity, have interestingly short timescales for the sedime...
This viewgraph presentation describes neutron stars and thermonuclear x ray bursts. The contents inc...
Observations of Type I X-ray bursts have long been taken as evidence that the sources are neutron st...
Observations of thermonuclear (Type I) X-ray bursts from neutron stars in low mass X-ray binaries (L...
Since the advent of powerful new X-ray observatories, NASA's Rossi X-ray Timing Explorer (RXTE), the...
Neutron stars are the most compact stars that can be directly observed, which makes them ideal labor...
Neutron stars offer a unique environment in which to develop and test theories of the strong force. ...
Results of various observations of common type I X-ray bursts are discussed with respect to the theo...
I review our understanding of the thermonuclear instabilities on accreting neutron stars that produc...
Burst oscillations, a phenomenon observed in a significant fraction of Type I (thermonuclear) X-ray ...
Observational evidence has been accumulating that thermonuclear X-ray bursts ignited on the surface ...
Unstable thermonuclear burning on the surface of accreting neutron stars is commonly observed as t...
Neutron stars (NS) are the most compact objects that can be directly observed. They can be used to s...
Analysis of observations of the X-ray emission produced by accreting neutron stars with millisecond ...
© 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society....
Neutron stars, with their strong surface gravity, have interestingly short timescales for the sedime...