Kilohertz oscillations in 4U 0614+091 and other LMXBs

Details Kilohertz oscillations in 4U 0614+091 and other LMXBs Kilohertz oscillations in 4U 0614+091 and other LMXBs

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410..697f&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 697-702 (1997).

Computer Science

X-Ray Binaries, Neutron Stars, Accretion And Accretion Disks

Scientific paper

Strong oscillations near 1000 Hz have been discovered in a number of low mass x-ray binaries with NASA's Rossi X-Ray Timing Explorer. Their behavior should ultimately lead us to a better understanding of the accretion dynamics and the fundamental properties of the neutron star itself. Here we summarize the known properties of fast QPOs, focusing on results from the source 4U 0614+091. We highlight some of the aspects yet to be explored.

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