Kilohertz Quasi-Periodic Oscillations and Strong Field Gravity in X-Ray Binaries

Research output: Chapter in Book/Report/Conference proceedingConference contributionAcademic

Abstract

Kilohertz quasi-periodic oscillations (kHz QPOs) are probably caused by matter in Keplerian orbit at some preferred radius in the accretion disc around a compact star. In a given source, QPO frequencies can drift by a few hundred Hz following changes of the inner disc radius; but the disc cannot move closer to the star than the radius of the innermost stable circular orbit (ISCO) predicted by general realtivity, hence the kHz QPO frequencies must be limited by some maximum frequency.
Original languageEnglish
Title of host publicationThe Ninth Marcel Grossmann Meeting
Subtitle of host publicationOn Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories (In 3 Volumes)
EditorsVahe G. Gurzadian, Robert T. Jantzen, Remo Rufini
PublisherWorld Scientific Publishing
Pages2218-2219
ISBN (Electronic)978-981-4488-49-5
ISBN (Print)978-981-238-010-4
DOIs
Publication statusPublished - 1-Dec-2002
Externally publishedYes
EventThe Ninth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories - The University of Rome ‘La Sapienza’, Rome, Italy
Duration: 2-Jul-20028-Jul-2002

Conference

ConferenceThe Ninth Marcel Grossmann Meeting
Country/TerritoryItaly
CityRome
Period02/07/200208/07/2002

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