Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..431..371c&link_type=abstract
Accretion processes in astrophysical systems: Some like it hot! - eigth astrophysics conference. AIP Conference Proceedings, Vo
Astronomy and Astrophysics
Astrophysics
X-Ray Binaries, Neutron Stars, Accretion And Accretion Disks, Nuclear Matter Aspects Of Neutron Stars
Scientific paper
The remarkable discovery of kilohertz quasi-periodic brightness oscillations (QPOs) in the accretion-powered emission from some sixteen neutron-star low-mass X-ray binary systems has led to much speculation about and theoretical modeling of the origin of these oscillations. It has also led to intense study of the implications that these QPOs have for the properties of neutron stars and of the accretion flow onto them. In this review we describe the strengths and weaknesses of the models that have been proposed for the kilohertz QPOs observed in the accretion-powered emission. We conclude that beat-frequency models, and in particular the sonic-point model, are currently the most promising. If these models are correct, the kilohertz QPOs provide the strongest constraints to date on the masses and radii of neutron stars in low-mass X-ray binaries, and on the equation of state of the dense matter in all neutron stars.
No associations
LandOfFree
Models of kilohertz quasi-periodic brightness oscillations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Models of kilohertz quasi-periodic brightness oscillations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Models of kilohertz quasi-periodic brightness oscillations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1602193