The cooling phase of Type I X-ray bursts observed with RXTE in 4U 1820-30 does not follow the canonical F proportional to T-4 relationGarcia, F., Zhang, G. & Mendez, M., Mar-2013, In : Monthly Notices of the Royal Astronomical Society. 429, 4, p. 3266-3271 6 p.
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We analysed the complete set of bursts from the neutron star low-mass X-ray binary 4U 1820-30 detected with the Rossi X-ray Timing Explorer (RXTE). We found that all are photospheric radius expansion bursts, and have similar duration, peak flux and fluence. From the analysis of time-resolved spectra during the cooling phase of the bursts, we found that the relation between the bolometric flux and the temperature is very different from the canonical F proportional to T-4 relation which is expected if the apparent emitting area on the surface of the neutron star remains constant. The flux-temperature relation can be fitted using a broken power law, with indices nu(1) = 2.0 +/- 0.3 and nu(2) = 5.72 +/- 0.06. The departure from the F proportional to T-4 relation during the cooling phase of the X-ray bursts in 4U 1820-30 could be due to changes in the emitting area of the neutron star while the atmosphere cools down, variations in the colour-correction factor due to chemical evolution, or the presence of a source of heat, e.g. residual hydrogen nuclear burning, playing an important role when the burst emission ceases.
|Number of pages||6|
|Journal||Monthly Notices of the Royal Astronomical Society|
|Publication status||Published - Mar-2013|
- stars: individual: 4U 1820-30, stars: neutron, X-rays: binaries, X-rays: bursts, PHOTOSPHERIC RADIUS EXPANSION, QUASI-PERIODIC OSCILLATIONS, NEUTRON-STARS, TIMING-EXPLORER, THERMONUCLEAR BURST, INTERSTELLAR-MEDIUM, MASS, PROPAGATION, DISCOVERY, SUPEREXPANSION