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Michal Bursa

Researcher at Academy of Sciences of the Czech Republic

Publications -  76
Citations -  2529

Michal Bursa is an academic researcher from Academy of Sciences of the Czech Republic. The author has contributed to research in topics: Accretion (astrophysics) & Black hole. The author has an hindex of 22, co-authored 69 publications receiving 2229 citations. Previous affiliations of Michal Bursa include Max Planck Society.

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The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

Kirpal Nandra, +239 more
TL;DR: The Advanced Telescope for High Energy Astrophysics (Athena+) mission as discussed by the authors provides the necessary performance (e.g., angular resolution, spectral resolution, survey grasp) to address these questions and revolutionize our understanding of the Hot and Energetic Universe.
Proceedings ArticleDOI

eXTP: Enhanced X-ray Timing and Polarization mission

Shuang-Nan Zhang, +184 more
- 26 Jun 2016 - 
TL;DR: eXTP as discussed by the authors is a science mission designed to study the state of matter under extreme conditions of density, gravity and magnetism, which carries a unique and unprecedented suite of state-of-the-art scientific instruments enabling for the first time ever the simultaneous spectral-timing-polarimetry studies of cosmic sources in the energy range from 0.5-30 keV.
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Evidence for a 2:3 resonance in Sco X-1 kHz QPOs

TL;DR: In this article, it was shown that the two high frequency QPOs in Sco X-1 are, more often than not, approximately in the 2:3 frequency ratio familiar from studies of black hole candidates.
Journal ArticleDOI

Relativistic slim disks with vertical structure

TL;DR: In this paper, a scheme for incorporating vertical radiative energy transport into a fully relativistic, Kerr-metric model of optically thick, advective, transonic alpha disks was proposed.
Journal ArticleDOI

Relativistic slim disks with vertical structure

TL;DR: In this paper, a scheme for incorporating vertical radiative energy transport into a fully relativistic, Kerr-metric model of optically thick, advective, transonic alpha disks was proposed.