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 language | English |
---|---|
Title of host publication | The Ninth Marcel Grossmann Meeting |
Subtitle of host publication | On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories (In 3 Volumes) |
Editors | Vahe G. Gurzadian, Robert T. Jantzen, Remo Rufini |
Publisher | World Scientific Publishing |
Pages | 2218-2219 |
ISBN (Electronic) | 978-981-4488-49-5 |
ISBN (Print) | 978-981-238-010-4 |
DOIs | |
Publication status | Published - 1-Dec-2002 |
Externally published | Yes |
Event | The 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-2002 → 8-Jul-2002 |
Conference
Conference | The Ninth Marcel Grossmann Meeting |
---|---|
Country/Territory | Italy |
City | Rome |
Period | 02/07/2002 → 08/07/2002 |