External Organisations

  • McGill University, Canada
  • International Space Science Institute, Switzerland

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Description

Thermonuclear flashes on accreting neutron stars, observed as Type I X-ray bursts, offer a powerful probe of the conditions inside the dense interior of the neutron star. We propose a combined observational and theoretical effort to understand the lightcurves, energetics and ignition conditions of long duration X-ray bursts, using them to measure the temperature of the neutron star interior, and to constrain the mass and radius of neutron stars from the spectrum of Type I X-ray bursts. These approaches give complementary information about the neutron star interior, constraining the uncertain physics of dense matter.
StatusFinished
Effective start/end date01/01/201112/07/2014

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ID: 155498829