Prohlížení Acta Polytechnica CTU Proceedings. 2014, vol. 1, no. 1 dle názvu
Zobrazují se záznamy 24-43 z 62
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Final Remarks
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014) -
First Hints of Pressure Waves in a Helical Extragalactic Jet: S5 0836+710
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)One of the open questions in extragalactic jet Astrophysics is related to the nature of the observed radio jet, namely whether it traces a pattern or the flow structure itself. In this paper I summarize the evidence collected ... -
Forty Years of X-Raying Narrow-Line Seyfert 1 Galaxies
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)Forty years after the discovery of Narrow-Line Seyfert 1 Galaxies (NLS1s), and 20 years since the discovery of the remarkable ultrasoft soft X-ray emissions of NLS1s, strategic publications improved the understanding of ... -
Fullerenes, PAHs, Amino Acids and High Energy Astrophysics
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)We present theoretical, observational and laboratory work on the spectral properties of fullerenes and hydrogenated fullerenes. Fullerenes in its various forms (individual, endohedral, hydrogenated, etc.) can contribute ... -
Gamma-rays, Neutrinos and Particle Astronomy as Messengers of the Universe
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)Observations of charged cosmic-rays, γ-rays and neutrino are possible thanks to the availability of new detectors coming from technologies typical of experimental particle physics. In conjunction with more traditional ... -
Gravitational Waves and Dark Energy
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)The idea that dark energy is gravitational waves may explain its strength and its time-evolution. A possible concept is that dark energy is the ensemble of coherent bursts (solitons) of gravitational waves originally ... -
HAVmS: Highly Available Virtual Machine Computer System Fault Tolerant with Automatic Failback and Close to Zero Downtime
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)In scientic computing, systems often manage computations that require continuous acquisition of of satellite data and the management of large databases, as well as the execution of analysis software and simulation models ... -
High-Resolution X-Ray Spectroscopy of Galactic Supernova Remnants
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)High-resolution X-ray spectroscopy of Galactic supernova remnants (SNRs), based on grating spectrometers onboard XMM-Newton and Chandra, has been revealing a variety of new astrophysical phenomena. Broadened oxygen lines ... -
Highly Magnetized Accreting Pulsars: Are There Accreting Magnetars?
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)2S 0114+650, GX 301-2, IGR J16358-4726, X Per, 4U 2206+54, SXP 1062, and 3A 1954+319 are thought to possess high magnetic elds. They have recently been named accreting magnetars, or highly magnetized accreting pulsars. In ... -
Latest Results from the Fermi Gamma-Ray Telescope
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)Can we learn about New Physics with astronomical and astro-particle data? Since its launch in 2008, the Large Area Telescope, onboard of the Fermi Gamma-ray Space Telescope, has detected the largest amount of gamma rays ... -
LHC, Astrophysics and Cosmology
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)In this paper we discuss the impact on cosmology of recent results obtained by the LHC (Large Hadron Collider) experiments in the 2011-2012 runs, respectively at √s = 7 and 8 TeV. The capital achievement of LHC in this ... -
Magnetorotational Explosions of Core-Collapse Supernovae
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)Core-collapse supernovae are accompanied by formation of neutron stars. The gravitation energy is transformed into the energy of the explosion, observed as SN II, SN Ib,c type supernovae. We present results of 2-D MHD ... -
Mass Accretion Processes in Young Stellar Objects: Role of Intense Flaring Activity
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)According to the magnetospheric accretion scenario, young low-mass stars are surrounded by circumstellar disks which they interact with through accretion of mass. The accretion builds up the star to its nal mass and is ... -
Modelling the Multifrequency SED of AGN Candidates among the Unidentied EGRET and Fermi Gamma-Ray Sources
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)Of the 271 sources in the 3rd EGRET catalogue, 131 were reported as unidentied, i.e. not associated with any particular class of point source in the sky. Since the largest fraction of the EGRET sources were extragalactic, ... -
Multi-Frequency Study of the SZ Effect in Cosmic Structures
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)The Sunyaev-Zel’dovich effect (SZE) is a relevant probe for cosmology and astrophysics. A multi-frequency approach to study the SZE in cosmic structures turns out to be crucial in the use of this probe for astrophysics and ... -
Multi-Wavelength View of Supernova Remnants
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)This contribution gives a very short overview on the emission of supernova remnants and the processes that are responsible for both the thermal and non-thermal origins of the emission, typically observed in radio, X-rays, ... -
Multifrequency Behaviour of the Gamma-Ray Binary System PSR B1259-63: Modelling the FERMI Flare
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)This paper presents a brief overview of the multifrequency properties of the gamma-ray binary system PSR B1259-63 from radio to very high energy gamma-rays. A summary is also presented of the various models put forward to ... -
Multiscale Modeling of Astrophysical Jets
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)We are developing the capability for a multi-scale code to model the energy deposition rate and momentum transfer rate of an astrophysical jet which generates strong plasma turbulence in its interaction with the ambient ... -
Old and New from Multifrequency Astrophysics
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)In this short review paper we comment on some the most important steps that have been made in the past decades for a better understanding of the physics governing our Universe. The results we discuss come from the many ... -
Origin of X-ray Spectral Variation and the Seemingly Broad Iron-Line Spectral Feature in Seyfert Galaxies
(České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)We present systematic X-ray data analysis of the Seyfert galaxies observed by Suzaku to study origin of their hard X-ray (2 - 40 keV) variations. In particular, we examine if the "Variable Partial Covering (VPC) model" ...