New Observational Results On The Probable Marginally Stable Nuclear Burning On Neutron Stars.

Details New Observational Results On The Probable Marginally Stable Nuclear Burning On Neutron Stars. New Observational Results On The Probable Marginally Stable Nuclear Burning On Neutron Stars.

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0760d&link_type=abstract

American Astronomical Society, HEAD meeting #9, #7.60; Bulletin of the American Astronomical Society, Vol. 38, p.359

Astronomy and Astrophysics

Astronomy

Scientific paper

We will report a detailed study of the timing and spectral characteristics of the millihertz quasi-periodic oscillations observed in the persistent source 4U 1636-53.
These phenomena are very likely due to a marginally stable nuclear burning on the neutron star surface. If confirmed, this would be the first time that quasi-periodic variability in the persistent X-ray flux is identified with a process on the neutron star surface rather than the accretion disk.

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