The Rising Phase of X-Ray Bursts from MXB:1728-34 - Constraints on the Spreading of Thermonuclear Flashes Over the Surface of the Neutron Star

Details The Rising Phase of X-Ray Bursts from MXB:1728-34 - Constraints on the Spreading of Thermonuclear Flashes Over the Surface of the Neutron Star The Rising Phase of X-Ray Bursts from MXB:1728-34 - Constraints on the Spreading of Thermonuclear Flashes Over the Surface of the Neutron Star

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.245p..31d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 245, NO. 1/JUL1, P. 31P, 1990

Astronomy and Astrophysics

Astronomy

10

Scientific paper

We present the results of the analysis of the rising phase of two X-ray bursts from MXB 1728-34. We find that the spectra can be fitted best by a blackbody, the emission area of which rises rapidly to a constant value before the peak of the burst is reached. This result is interpreted as placing a limit of 0.1 s on the time taken for the thermonuclear flash to spread over the surface of the neutron star.

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