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Showing 1 to 8 of 8 for “"X-ray bursts"”.

  1. Millisecond oscillations during thermonuclear X-ray bursts

    … trains detected in a search of 159 thermonuclear bursts from eight neutron star X-ray binaries observed with the Rossi X-ray Timing Explorer. I use all data that were public as of September 2001. The frequencies of the oscillations are uniformly distributed between 270-620 Hz, and are nearly …

    mit Repository record for Millisecond oscillations during thermonuclear X-ray bursts (opens in a new tab)

  2. Type I X-ray bursts as probes of the neutron star accretion flow

    Neutron stars in low-mass X-ray binaries frequently exhibit Type I X-ray bursts caused by unstable nuclear burning of accreted matter on the neutron star surface. X-ray bursts offer the opportunity to constrain the neutron star radii and masses and hence the equation of state of one of the densest …

    gatech Repository record for Type I X-ray bursts as probes of the neutron star accretion flow (opens in a new tab)

  3. Lifetimes of states in 19Ne above the 15O+ alpha threshold

    … stellar environments such as supernovae, X-ray bursts, novae etc. and nuclear data are important in the interpretation of these phenomena. When carbon, nitrogen and oxygen isotopes are present in substantial quantities in a star of sufficient mass, the fusion of four hydrogen nuclei to form …

    ubc Repository record for Lifetimes of states in 19Ne above the 15O+ alpha threshold (opens in a new tab)

  4. Astrophysical signatures of neutron stars in compact binaries and experimental improvements on gravitational-wave detectors

    … of super-Eddington winds launched in type-I X-ray bursts at the surface of a NS. We show that freshly synthesized heavy elements can be exposed by the wind and will dominate the composition at the photosphere after ~ 1 s. This may create detectable absorption edges in burst spectra and explain …

    mit Repository record for Astrophysical signatures of neutron stars in compact binaries and experimental improvements on gravitational-wave detectors (opens in a new tab)

  5. Accretion- and nuclear-powered phenomena in neutron stars with millisecond spin periods

    "Analysis of observations of the X-ray emission produced by accreting neutron stars with millisecond spin periods can provide important information about the masses M and radii R of neutron stars, thereby yielding uniquely valuable information about the still uncertain properties of cold matter at …

    uiuc Repository record for Accretion- and nuclear-powered phenomena in neutron stars with millisecond spin periods (opens in a new tab)

  6. Development of a Single-Crystal X-ray Spectropolarimeter and Application to Wire-Array Z-pinches

    … usually inferred from the observation of hard x-ray bursts. Spectroscopy is the way to diagnose plasmas, and because anisotropies such as electron beams can lead to the partial polarization of the emitted radiation, polarization spectroscopy, or spectropolarimetry, can be used to diagnose these …

    unr Repository record for Development of a Single-Crystal X-ray Spectropolarimeter and Application to Wire-Array Z-pinches (opens in a new tab)

  7. Observational and evolutionary studies of neutron star X-ray binaries

    … and evolutionary studies of neutron stars in X-ray binary systems. A variety of topics are discussed, which are all related by a single scientific theme, namely, helping to set constraints on the mass-radius relation of neutron stars, and hence on their equations of state (EOS). In Chapter 1 we …

    mit Repository record for Observational and evolutionary studies of neutron star X-ray binaries (opens in a new tab)

  8. X-ray spectroscopy of neutron star low-mass X-ray binaries

    … of topics relating to neutron star lowmass X-ray binaries (LMXBs) and utilize spectral information from X-ray observations to further our understanding of these sources. First, I give an overview of important X- ray astrophysics relevant to the work I present in subsequent chapters, as well as …

    mit Repository record for X-ray spectroscopy of neutron star low-mass X-ray binaries (opens in a new tab)