SRG/ART-XC, Swift, NICER, and NuSTAR study of different states of the transient X-ray pulsar MAXI J0903-531

Tsygankov, S.S.; Molkov, S.V.; Doroshenko, V.; Mushtukov, A.; Mereminskiy, I.A.; Semena, A.N.; Thalhammer, P.; Wilms, J.; Lutovinov, A.A.

doi:10.1051/0004-6361/202141821

SRG/ART-XC, Swift, NICER, and NuSTAR study of different states of the transient X-ray pulsar MAXI J0903-531

Author(s):: Tsygankov, S.S.; Molkov, S.V.; Doroshenko, V.; Mushtukov, A.; Mereminskiy, I.A.; Semena, A.N.; Thalhammer, P.; Wilms, J.; Lutovinov, A.A.

Published: 2022
Publication type: Article / Letter to editor

AccretionAccretion disksMagnetic fieldsX-rays - binariesStars - neutronPulsars - individual - MAXI J0903-531Radiative transferAstrophysics - high energy astrophysical phenomena

Date issued: 2022
Language: English
Is part of: Astronomy & Astrophysics (2022), A45
hdl: 1887/3562548
doi: 10.1051/0004-6361/202141821
URL: https://ui.adsabs.harvard.edu/abs/2022A&A...661A..45T

SRG/ART-XC, Swift, NICER, and NuSTAR study of different states of the transient X-ray pulsar MAXI J0903-531

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