A Transition Discovered in the Subcritical Regime of 1A 0535+262

We present NICER observations of the accreting X-ray pulsar 1A 0535+262 during its faint state (≲6 × 10 ^36 erg s ^−1 ), observed in several type I and type II outbursts. We discovered a transition of temporal and spectral properties around the luminosity L _t = 3.3 × 10 ^35 erg s ^−1 , below which...

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Main Authors: Hua Xiao, Long Ji
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad23cd
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author Hua Xiao
Long Ji
author_facet Hua Xiao
Long Ji
author_sort Hua Xiao
collection DOAJ
description We present NICER observations of the accreting X-ray pulsar 1A 0535+262 during its faint state (≲6 × 10 ^36 erg s ^−1 ), observed in several type I and type II outbursts. We discovered a transition of temporal and spectral properties around the luminosity L _t = 3.3 × 10 ^35 erg s ^−1 , below which spectra are relatively soft and the pulse profiles have only a narrow peak. The spectra are harder and a secondary hump gradually appears in the pulse profiles when L ≳ L _t . We discuss possible physical mechanisms for this transition, including different Comptonization seed photons, the disappearance of gas shocks on the neutron star surface, and the combination of plasma and vacuum polarization effects.
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spelling doaj.art-2ff9d7a410434a95bf0cf691f5a8e50c2024-02-28T09:17:32ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-0196314210.3847/1538-4357/ad23cdA Transition Discovered in the Subcritical Regime of 1A 0535+262Hua Xiao0https://orcid.org/0009-0004-1288-4912Long Ji1https://orcid.org/0000-0001-9599-7285School of Physics and Astronomy, Sun Yat-sen University , Zhuhai 519082, People’s Republic of China ; jilong@mail.sysu.edu.cnSchool of Physics and Astronomy, Sun Yat-sen University , Zhuhai 519082, People’s Republic of China ; jilong@mail.sysu.edu.cnWe present NICER observations of the accreting X-ray pulsar 1A 0535+262 during its faint state (≲6 × 10 ^36 erg s ^−1 ), observed in several type I and type II outbursts. We discovered a transition of temporal and spectral properties around the luminosity L _t = 3.3 × 10 ^35 erg s ^−1 , below which spectra are relatively soft and the pulse profiles have only a narrow peak. The spectra are harder and a secondary hump gradually appears in the pulse profiles when L ≳ L _t . We discuss possible physical mechanisms for this transition, including different Comptonization seed photons, the disappearance of gas shocks on the neutron star surface, and the combination of plasma and vacuum polarization effects.https://doi.org/10.3847/1538-4357/ad23cdAccretionHigh mass x-ray binary starsPulsars
spellingShingle Hua Xiao
Long Ji
A Transition Discovered in the Subcritical Regime of 1A 0535+262
The Astrophysical Journal
Accretion
High mass x-ray binary stars
Pulsars
title A Transition Discovered in the Subcritical Regime of 1A 0535+262
title_full A Transition Discovered in the Subcritical Regime of 1A 0535+262
title_fullStr A Transition Discovered in the Subcritical Regime of 1A 0535+262
title_full_unstemmed A Transition Discovered in the Subcritical Regime of 1A 0535+262
title_short A Transition Discovered in the Subcritical Regime of 1A 0535+262
title_sort transition discovered in the subcritical regime of 1a 0535 262
topic Accretion
High mass x-ray binary stars
Pulsars
url https://doi.org/10.3847/1538-4357/ad23cd
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