Issue |
A&A
Volume 648, April 2021
First science highlights from SRG/eROSITA
|
|
---|---|---|
Article Number | A39 | |
Number of page(s) | 10 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/202040145 | |
Published online | 09 April 2021 |
Observations of Her X-1 in low states during SRG/eROSITA all-sky survey
1
Moscow State University, Sternberg Astronomical Institute,
119234
Moscow,
Russia
e-mail: shakura@sai.msu.ru
2
Kazan Federal University,
420008
Kazan,
Russia
3
Space Research Institute of the Russian Academy of Sciences,
117997
Moscow,
Russia
4
Max-Planck-Institut für Astrophysik (MPA),
Karl-Schwarzschild-Str 1,
85741
Garching, Germany
Received:
16
December
2020
Accepted:
20
February
2021
eROSITA (extended ROentgen Survey with an Imaging Telescope Array) instrument onboard the Russian-German ‘Spectrum-Roentgen-Gamma’ (SRG) mission observed the Her X-1/HZ Her binary system in multiple scans over the source during the first and second SRG all-sky surveys. Both observations occurred during a low state of the X-ray source when the outer parts of the accretion disk blocked the neutron star from view. The orbital modulation of the X-ray flux was detected during the low states. We argue that the detected X-ray radiation results from scattering of the emission of the central source by three distinct regions: (a) an optically thin hot corona with temperature ~(2−4) × 106 K above the irradiated hemisphere of the optical star; (b) an optically thin hot halo above the accretion disk; and (c) the optically thick cold atmosphere of the optical star. The latter region effectively scatters photons with energies above 5–6 keV.
Key words: accretion, accretion disks / binaries : close / stars: neutron / X-rays: binaries
© ESO 2021
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