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Timing of accreting neutron stars with future X-ray instruments: towards new constraints on dense matter equation of state
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SYSNO ASEP 0581900 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Timing of accreting neutron stars with future X-ray instruments: towards new constraints on dense matter equation of state Author(s) Karas, Vladimír (ASU-R) RID, ORCID
Klimovičová, K. (CZ)
Lančová, D. (CZ)
Štolc, Marcel (ASU-R)
Svoboda, Jiří (ASU-R) RID, ORCID
Török, G. (CZ)
Matuszková, M. (CZ)
Šrámková, E. (CZ)
Šprňa, R. (CZ)
Urbanec, M. (CZ)Source Title Contributions of the Astronomical Observatory Skalnaté Pleso. - : Slovenská akadémia vied - ISSN 1335-1842
Roč. 53, č. 4 (2023), s. 175-190Number of pages 16 s. Publication form Online - E Language eng - English Country SK - Slovakia Keywords black holes ; neutron stars ; X-rays binaries OECD category Astronomy (including astrophysics,space science) R&D Projects GX21-06825X GA ČR - Czech Science Foundation (CSF) Method of publishing Open access Institutional support ASU-R - RVO:67985815 UT WOS 001141834600007 EID SCOPUS 85184768258 DOI 10.31577/caosp.2023.53.4.175 Annotation We provide a progress report on the Czech contribution to the eXTP science. We report on our simulation results performed in Opava (Institute of Physics of the Silesian University in Opava) and Prague (Astronomical Institute of the Czech Academy of Sciences), where the advanced timing capabilities of the satellite have been assessed for bright X-ray binaries that contain an accreting neutron star (NS) and exhibit the quasi-periodic oscillations. Both stellar-mass, supermassive, and tentative intermediate-mass black holes can be included in the program portfolio.
Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2024 Electronic address https://hdl.handle.net/11104/0350045
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