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A polarimetrically oriented X-ray stare at the accreting pulsar EXO 2030+375

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00574440" target="_blank" >RIV/67985815:_____/23:00574440 - isvavai.cz</a>

  • Result on the web

    <a href="https://hdl.handle.net/11104/0345205" target="_blank" >https://hdl.handle.net/11104/0345205</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/202346581" target="_blank" >10.1051/0004-6361/202346581</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    A polarimetrically oriented X-ray stare at the accreting pulsar EXO 2030+375

  • Original language description

    Accreting X-ray pulsars (XRPs) are presumed to be ideal targets for polarization measurements, as their high magnetic field strength is expected to polarize the emission up to a polarization degree of similar to 80%. However, such expectations are being challenged by recent observations of XRPs with the Imaging X-ray Polarimeter Explorer (IXPE). Here, we report on the results of yet another XRP, namely, EXO 2030+375, observed with IXPE and contemporarily monitored with Insight-HXMT and SRG/ART-XC. In line with recent results obtained with IXPE for similar sources, an analysis of the EXO 2030+375 data returns a low polarization degree of 0%-3% in the phase-averaged study and a variation in the range of 2%-7% in the phase-resolved study. Using the rotating vector model, we constrained the geometry of the system and obtained a value of similar to 60 degrees for the magnetic obliquity. When considering the estimated pulsar inclination of similar to 130 degrees, this also indicates that the magnetic axis swings close to the observer's line of sight. Our joint polarimetric, spectral, and timing analyses hint toward a complex accreting geometry, whereby magnetic multipoles with an asymmetric topology and gravitational light bending significantly affect the behavior of the observed source.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2023

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

    1432-0746

  • Volume of the periodical

    675

  • Issue of the periodical within the volume

    July

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    10

  • Pages from-to

    A29

  • UT code for WoS article

    001023752300009

  • EID of the result in the Scopus database

    2-s2.0-85164539143