A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Inertial oscillation modes of an inclined dipolar magnetosphere as a source of band-limited noise in X-ray pulsars
Tekijät: Pavel Abolmasov , Anton Biryukov
Kustantaja: OXFORD UNIV PRESS
Julkaisuvuosi: 2020
Lehti: Monthly Notices of the Royal Astronomical Society
Tietokannassa oleva lehden nimi: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Lehden akronyymi: MON NOT R ASTRON SOC
Vuosikerta: 496
Numero: 1
Aloitussivu: 13
Lopetussivu: 18
Sivujen määrä: 6
ISSN: 0035-8711
DOI: https://doi.org/10.1093/mnras/staa1544
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/49824570
Magnetic fields of strongly magnetized stars can trap conducting matter due to frozen-in condition. In the force-free regime, the motion of the matter along the field lines may be considered in the 'bead on a wire' approximation. Such a motion, if gravity and centrifugal forces are taken into account, has equilibrium points, some of which are stable. In most cases, stability is possible in about several per cent of the possible locations. Corresponding oscillation frequencies span the range from zero to root 3 of the spin frequency. We suggest that this variability mode may be excited in some X-ray pulsars during the outbursts and create the peaked broad-band noise component near the break frequency in the power density spectrum, as well as produce some of the quasi-periodic oscillation features in this frequency range. Existence of this variability does not require any changes in mass accretion rate and involves only a small amount of matter infiltrating from the disc and magnetic flow due to interchange instabilities.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
