National Repository of Grey Literature 9 records found  Search took 0.01 seconds. 
Modelování dichotomie polarizace záření aktivních galaktických jader
Goosmann, René
I present polarization modelling of Active Galactic Nuclei in the optical/UV range. The modelling is conducted using the Monte-Carlo radiative transfer code Stokes, which self-consistently models the polarization signature of a complex model arrangement for an active nucleus.
Modulace HFQPO
Bursa, Michal
We study strong-gravity effects on modulation of radiation emerging from accreting compact objects as a possible mechanism for flux modulation in QPOs.
O vzájemných vazbách mezi kHz QPOs
Török, G. ; Bursa, Michal ; Horák, Jiří ; Stuchlík, Z. ; Bakala, P.
We further investigate the issue of kHz QPO frequency ratios in neutron star low mass X-ray binaries. In this note we report on recent analysis of occurrences and properties of kHz QPOs in the source 4U1636-53. Assuming that kHz QPOs occur in pairs whose frequencies are linearly correlated, we find a prominent frequency range that separates upper and lower QPO observations.
Nestabilita akrečního disku jako zdroj energie pro kvaziperiodické oscilace
Horák, Jiří
We discuss a scenario, in which the energy for quasi-periodic oscillations comes from instabilities of the accretion disk. We demonstrate this mechanism on the interaction among stable and unstable modes of oscillations in slender accretion tori. In our model, the unstable non-axisymmetric corotation modes are nonlinearly coupled to stable acoustic modes of torus oscillations. The increasing energy of corotation modes is advected to the acoustic modes by the means of parametric instability. The stable modes may reach substantial amplitudes even if they are damped according to the linear theory.
Opticka spektroskopie Cyg X-1
Hadrava, Petr
The star HDE 226868 known as an optical counterpart of the black hole candidate Cyg X-1 has been observed in H_alpha region using spectrograph at Ondrejov 2-m telescope. The orbital parameters are determined from HeI-line by means of the author's method of Fourier disentangling. Preliminary results are also presented of disentangling the H_alpha-line into a P-Cyg profile of the (optical) primary and an emission profile of the circumstellar matter (and a telluric component).
O existenci haló orbit v Kerrových-Newmanových prostoročasech
Kovář, J. ; Stuchlík, Z. ; Karas, Vladimír
We discuss existence of halo orbits in Kerr–Newman spacetimes.
Záblesky ze spirálních vln ovlivněné efektem čočkování a časového zpoždění?
Karas, Vladimír ; Dovčiak, Michal ; Eckart, A. ; Meyer, L.
We examine physics of flares from spiral waves by lensing and time-delay amplification.
Změna primárního a reprocesovaného záření v modelu záblesků a skvrn
Dovčiak, Michal ; Karas, Vladimír ; Matt, G. ; Goosmann, René
We study variation of the primary and reprocessed radiation in the flare-spot model.

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