Timing of accreting neutron stars with future X-ray instruments: towards new constraints on dense matter equation of state

0581900 - ASÚ 2024 RIV SK eng J - Článek v odborném periodiku
Karas, Vladimír - Klimovičová, K. - Lančová, D. - Štolc, Marcel - Svoboda, Jiří - Török, G. - Matuszková, M. - Šrámková, E. - Šprňa, R. - Urbanec, M.
Timing of accreting neutron stars with future X-ray instruments: towards new constraints on dense matter equation of state.
Contributions of the Astronomical Observatory Skalnaté Pleso. Roč. 53, č. 4 (2023), s. 175-190. ISSN 1335-1842. E-ISSN 1336-0337
Grant CEP: GA ČR(CZ) GX21-06825X
Institucionální podpora: RVO:67985815
Klíčová slova: black holes * neutron stars * X-rays binaries
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 0.5, rok: 2022
Způsob publikování: Open access

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.

Trvalý link: https://hdl.handle.net/11104/0350045