UV and X-ray pulse amplitude variability in the transitional millisecond pulsar PSR J1023+0038
نویسندگان
چکیده
The transitional millisecond pulsar PSR J1023+0038 is the first discovered to emit UV and optical pulses. Here we present results of X-ray phase-resolved timing analysis observations performed with Hubble Space Telescope, XMM-Newton, NuSTAR satellites between 2014 2021. Ultraviolet pulsations are detected in high luminosity mode disappear during low flaring modes, similar what observed band. In mode, find variability both pulse amplitudes. root mean square pulsed amplitude band ranges from ~2.1% down ~0.7%, while it oscillates interval 5.5–12% As also band, this not correlated orbital phase. Notwithstanding rather statistics, have marginal evidence that variations do occur simultaneously bands. When decreases below detection threshold, no significant variation observed. These oscillations could be caused by small random mass accretion rate leading a size intra-binary shock region. Finally, flux spectral distribution well fitted using power-law relation form ν F ∼ν 0.4 . This supports hypothesis common physical mechanism underlying X-ray, UV, emissions J1023+0038.
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ژورنال
عنوان ژورنال: Astronomy and Astrophysics
سال: 2022
ISSN: ['0004-6361', '1432-0746']
DOI: https://doi.org/10.1051/0004-6361/202243180