• A Review of Astrophysical Jets 

      Autor: Beall, James H.
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      Astrophysical jets are ubiquitous: this simple statement has become a commonplace over the last three decades and more as a result of observing campaigns using detectors sensitive from radio to gamma-ray energies. During ...
    • The World Space Observatory - Ultraviolet (WSO-UV) Space Telescope; Status Update in 2013 

      Autor: Gómez de Castro, Ana I.; Shustov, Boris; Sachkov, Mikhail
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      This is a short primer and a brief update on the status of the World Space Observatory-Ultraviolet (WSO-UV) project dated in May 2013. WSO-UV is a 170m primary space telescope equipped for ultraviolet imaging and spectroscopy ...
    • ARGO-YBJ: Highlights and Prospects 

      Autor: Di Sciascio, Giuseppe
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      The ARGO-YBJ experiment has been in stable data taking for 5 years at the YangBaJing Cosmic Ray Laboratory (Tibet, P.R. China, 4300 m a.s.l., 606 g/cm2). With a duty-cycle greater than 86% the detector collected about 51011 ...
    • Multifrequency Behaviour of the Gamma-Ray Binary System PSR B1259-63: Modelling the FERMI Flare 

      Autor: van Soelen, Brian; Meintjes, Pieter J.
      (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 ...
    • Old and New from Multifrequency Astrophysics 

      Autor: Giovannelli, Franco; Sabau-Graziati, Lola
      (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 ...
    • LHC, Astrophysics and Cosmology 

      Autor: Auriemma, Giulio
      (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 ...
    • AGN/Starburst Connection 

      Autor: Sani, Eleonora
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      Two main physical processes characterize the activity in the nuclear region of active galaxies: an intense star formation (starburst, SB) and an Active Galactic Nucleus (AGN). While the existence of a starburst-AGN connection ...
    • Gamma-rays, Neutrinos and Particle Astronomy as Messengers of the Universe 

      Autor: Spurio, Maurizio
      (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 ...
    • Latest Results from the Fermi Gamma-Ray Telescope 

      Autor: Morselli, Aldo
      (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 ...
    • Forty Years of X-Raying Narrow-Line Seyfert 1 Galaxies 

      Autor: Boller, Thomas
      (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 ...
    • Star Formation as Seen by Low Mass Stars 

      Autor: Panagia, Nino; De Marchi, Guido
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      Using the Hubble Space Telescope (HST) we have characterised and compared the physical properties of a large sample of pre-main sequence (PMS) stars spanning a wide range of masses (0:5 - 4Mʘ), metallicities (0:1 - 1 Zʘ) ...
    • Auger Highlights 

      Autor: Castellina, Antonella
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      The Pierre Auger Observatory has been designed to investigate the origin and nature of the ultra high energy cosmic rays using a hybrid detection technique. A review of selected results is presented, with the emphasis given ...
    • Electron Acceleration in Supernovae and Millimeter Perspectives 

      Autor: Maeda, Keiichi
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      Supernovae launch a strong shock wave by the interaction of the expanding ejecta and surrounding circumstellar matter (CSM). At the shock, electrons are accelerated to relativistic speed, creating observed synchrotron ...
    • V2282 Sgr Revisited 

      Autor: Nesci, Roberto; Rossi, Corinne; Frasca, Antonio; Marilli, Ettore; Persi, Paolo; Cornero, Nicola
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      The nature of V2282 Sgr is examined on the basis of several multiband observations: a 20 years long I-band light curve of V2282 Sgr obtained from archive photographic plates of the Asiago and Catania Observatories; a CCD ...
    • Cosmological Evolution of the Central Engine in High-Luminosity, High-Accretion Rate AGN 

      Autor: Guainazzi, Matteo
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      In this paper I discuss the status of observational studies aiming at probing the cosmological evolution of the central engine in high-luminosity, high-accretion rate Active Galactic Nuclei (AGN). X-ray spectroscopic ...
    • The Formation of Massive Stars: from Herschel to Near-Infrared 

      Autor: Persi, Paolo; Tapia, Mauricio
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      We have studied a number of selected high mass star forming regions, including high resolution near-infrared broad- and narrow-band imaging, Herschel (70, 160, 250, 350 and 500 μm) and Spitzer (3.6, 4.5, 5.8 and 8.0 m) ...
    • Gravitational Waves and Dark Energy 

      Autor: Biermann, Peter L.; Harms, Benjamin C.
      (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 ...
    • Be/X-Ray Binaries with Black Holes in the Galaxy and in the Magellanic Clouds 

      Autor: Ziolkowski, Janusz
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      I will start with the statistics indicating that the objects named in the title of my talk are either non-existing or very elusive to detect (not a single such object is known against 119 known Be/neutron star X-ray ...
    • Planck 2013 Cosmology Results: a Review 

      Autor: Rubino-Martín, José Alberto
      (České vysoké učení technické v PrazeCzech Technical University in Prague, 2014)
      This talk presents an overview of the cosmological results derived from the first 15.5 months of observations of the ESA’s Planck mission. These cosmological results are mainly based on the Planck measurements of the cosmic ...
    • Multi-Wavelength View of Supernova Remnants 

      Autor: Sasaki, Manami
      (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, ...