Production of QPOs in accreting neutron star systems

Details Production of QPOs in accreting neutron star systems Production of QPOs in accreting neutron star systems

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006adspr..38.2680m&link_type=abstract

Advances in Space Research, Volume 38, Issue 12, p. 2680-2683.

Physics

1

Scientific paper

Kilohertz QPOs have been detected from more than 20 neutron stars in low-mass X-ray binaries. Several different ideas have been proposed for their generation, involving resonances, magnetic interactions, and sharp transitions in the accretion flow. We show that although details are uncertain at this time, it is clear that the stellar magnetic field has a dynamic influence on the accretion flow. We also discuss the inferences about dense matter and strong gravity that can be drawn from all models, and the qualitative advances expected with a future X-ray timing mission.

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