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Table · dataset · 2026

Pulsar Vela X-1 Pulse-to-Pulse Approach

Listed in IVOA Registry (Virtual Observatory)

We investigated the long-term evolution of the cyclotron line energy, as well as the relationship between cyclotron line energy and luminosity in the high-mass X-ray binary Vela X-1, based on archival Swift/BAT monitoring from 2005 to 2024 and pulse-to-pulse analysis of nine NuSTAR observations from 2012 to 2024.

Description

Our results provide the first confirmation that the long-term decay of the harmonic line energy (E_cyc_,H) in Vela X-1 has ended.

We further report the first detection of a transient increase in E_cyc_,H between 2020 and 2023, which suggests a sudden and significant change in the magnetic field configuration or accretion geometry. In addition, E_cyc_,H shows slightly lower values at low luminosities and tends to flatten at higher luminosities, in the range of (0.13-1.21)x10^37^erg/s. The fundamental line energy (E_cyc_,F) exhibits no significant variation with time or luminosity, remaining stable at approximately 25keV.

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Stated by source
Gamma-Ray · Radio
Provenance · 1 source records, 9 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/706/a17515 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:gamma-raysource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:radiosource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0