This viewgraph presentation describes neutron stars and thermonuclear x ray bursts. The contents include: 1) Neutron Stars: why do we care?; 2) Thermonuclear Bursts: why do we care?; 3) Neutron Stars: Mass, Radius and Spin: a. Continuum Spectroscopy of Bursts b. Spectral Lines from Bursts c. Timing Properties of Bursts; 4) Neutron Star Atmosphere: Thermonuclear Flame Spreading; and 5) Future Prospects and Conclusions
Neutron stars represent the endpoint in stellar evolution for stars with initial masses between abou...
Thermonuclear (type-I) bursts arise from unstable ignition of accumulated fuel on the surface of neu...
Type I X-ray bursts are thermonuclear explosions that occur in the envelopes of accreting neutron st...
Studies of thermonuclear X-ray bursts can be very useful to constrain the spin rate, mass and radius...
Observations of Type I X-ray bursts have long been taken as evidence that the sources are neutron st...
Results of various observations of common type I X-ray bursts are discussed with respect to the theo...
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...
I review our understanding of the thermonuclear instabilities on accreting neutron stars that produc...
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 offer a unique environment in which to develop and test theories of the strong force. ...
Observations of thermonuclear (Type I) X-ray bursts from neutron stars in low mass X-ray binaries (L...
© 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society....
Unresolved issues involving neutron star binaries, pulsars, and burst sources are described. Attenti...
Neutron stars represent the endpoint in stellar evolution for stars with initial masses between abou...
Thermonuclear (type-I) bursts arise from unstable ignition of accumulated fuel on the surface of neu...
Type I X-ray bursts are thermonuclear explosions that occur in the envelopes of accreting neutron st...
Studies of thermonuclear X-ray bursts can be very useful to constrain the spin rate, mass and radius...
Observations of Type I X-ray bursts have long been taken as evidence that the sources are neutron st...
Results of various observations of common type I X-ray bursts are discussed with respect to the theo...
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...
I review our understanding of the thermonuclear instabilities on accreting neutron stars that produc...
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 offer a unique environment in which to develop and test theories of the strong force. ...
Observations of thermonuclear (Type I) X-ray bursts from neutron stars in low mass X-ray binaries (L...
© 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society....
Unresolved issues involving neutron star binaries, pulsars, and burst sources are described. Attenti...
Neutron stars represent the endpoint in stellar evolution for stars with initial masses between abou...
Thermonuclear (type-I) bursts arise from unstable ignition of accumulated fuel on the surface of neu...
Type I X-ray bursts are thermonuclear explosions that occur in the envelopes of accreting neutron st...