X-ray variability of transitional millisecond pulsars: a faint, stable, and fluctuating disc

X-ray variability of transitional millisecond pulsars: a faint, stable, and fluctuating disc

Transitional millisecond pulsars (tMSPs) have emerged in the last decade as a unique class of neutron stars at the crossroads between accretion- and rotation-powered phenomena. In their (sub-luminous) accretion disc state, with X-ray luminosities of order 1033-1034 erg s-1, they switch rapidly betwe...

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Bibliographic Details
Main Authors: De Marco, B. (Author), Linares, M. (Author), Van Der Klis, M. (Author), Wijnands, R. (Author)
Format: Article
Language:English
Published: Oxford University Press 2022
Subjects:
accretion, accretion discs
Accretion: accretion disks
Globular cluster: individual: (m28)
Globular clusters: individual
globular clusters: individual: (M28)
Luminance
Millisecond pulsars
Pulsar: individual: (PSR j1824-2452i, PSR j1023 + 0038, PSR j1227-4853)
Pulsars
pulsars: individual: (PSR J1824-2452I, PSR J1023 + 0038, PSR J1227-4853)
Pulsars:individual
stars: neutron
Stars: neutrons
X-ray: individual: (IGR j18245-2452, 2XMM j102347.6 + 003841, XSS j12270-4859)
X-rays: binaries
X-rays: Binaries
X-rays: individual
X-rays: individual: (IGR J18245-2452, 2XMM J102347.6 + 003841, XSS J12270-4859)
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