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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Format: | Article |
Language: | English |
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EDP Sciences
2014-01-01
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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. |
first_indexed | 2024-12-18T11:38:08Z |
format | Article |
id | doaj.art-3cbdd64112354301bceacccbac7b6be6 |
institution | Directory Open Access Journal |
issn | 2100-014X |
language | English |
last_indexed | 2024-12-18T11:38:08Z |
publishDate | 2014-01-01 |
publisher | EDP Sciences |
record_format | Article |
series | EPJ Web of Conferences |
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 |
work_keys_str_mv | AT blinovaaa oscillationsoftheboundarylayerandhighfrequencyqpos AT bachettim oscillationsoftheboundarylayerandhighfrequencyqpos AT romanovamm oscillationsoftheboundarylayerandhighfrequencyqpos |