Oscillations of the Boundary Layer and High-frequency QPOs

We observed persistent high-frequency oscillations of the boundary layer near an accreting, weakly-magnetized star in global 3D MHD simulations. The tilted dipole magnetic field is not strong enough to open a gap between the star and the disk. Instead, it forms a highly-wrapped azimuthal field near...

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Main Authors: Blinova A. A., Bachetti M., Romanova M. M.
Format: Article
Language:English
Published: EDP Sciences 2014-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20136405009
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author Blinova A. A.
Bachetti M.
Romanova M. M.
author_facet Blinova A. A.
Bachetti M.
Romanova M. M.
author_sort Blinova A. A.
collection DOAJ
description We observed persistent high-frequency oscillations of the boundary layer near an accreting, weakly-magnetized star in global 3D MHD simulations. The tilted dipole magnetic field is not strong enough to open a gap between the star and the disk. Instead, it forms a highly-wrapped azimuthal field near the surface of the star which slows down rotation of the disk matter, while a small tilt of the field excites oscillations of the boundary layer with a frequency below the Keplerian frequency. This mechanism may be responsible for the high-frequency oscillations in accreting neutron stars, white dwarfs and classical T Tauri stars.
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spelling doaj.art-3cbdd64112354301bceacccbac7b6be62022-12-21T21:09:28ZengEDP SciencesEPJ Web of Conferences2100-014X2014-01-01640500910.1051/epjconf/20136405009epjconf_mag2013_05009Oscillations of the Boundary Layer and High-frequency QPOsBlinova A. A.Bachetti M.Romanova M. M.We observed persistent high-frequency oscillations of the boundary layer near an accreting, weakly-magnetized star in global 3D MHD simulations. The tilted dipole magnetic field is not strong enough to open a gap between the star and the disk. Instead, it forms a highly-wrapped azimuthal field near the surface of the star which slows down rotation of the disk matter, while a small tilt of the field excites oscillations of the boundary layer with a frequency below the Keplerian frequency. This mechanism may be responsible for the high-frequency oscillations in accreting neutron stars, white dwarfs and classical T Tauri stars.http://dx.doi.org/10.1051/epjconf/20136405009
spellingShingle Blinova A. A.
Bachetti M.
Romanova M. M.
Oscillations of the Boundary Layer and High-frequency QPOs
EPJ Web of Conferences
title Oscillations of the Boundary Layer and High-frequency QPOs
title_full Oscillations of the Boundary Layer and High-frequency QPOs
title_fullStr Oscillations of the Boundary Layer and High-frequency QPOs
title_full_unstemmed Oscillations of the Boundary Layer and High-frequency QPOs
title_short Oscillations of the Boundary Layer and High-frequency QPOs
title_sort oscillations of the boundary layer and high frequency qpos
url http://dx.doi.org/10.1051/epjconf/20136405009
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