Results 71 to 80 of about 120,893 (256)
On Possible Reduction of Equilibrium Radius of a Neutron Star Influenced by Superstrong Magnetic Field
Advances in High Energy Physics, Volume 2012, Issue 1, 2012., 2012 Necessary condition for β‐decay suppression of a neutron in degenerate magnetized electron gas is formulated. Based on this, it is shown that, in superstrong magnetic field, equilibrium radius of a neutron star is approximately several times smaller than without the field influence. Therefore, we can make a prediction that in short‐period pulsars, such Vladimir V. Skobelev, C. Q. Gengwiley +1 more sourceThe specifics of pulsar radio emission
Open Astronomy, 2022 A characteristic property of pulsars is pulsed periodic radio emission, which has a high stability of periods. Despite the high stability of the emission periods of pulsars, monitoring the time of arrival of pulses (timing) shows the presence of ...Losovsky Boris Ya.doaj +1 more sourcePulsar‐Driven Jets in Supernovae, Gamma‐Ray Bursts, and the Universe
Advances in Astronomy, Volume 2012, Issue 1, 2012., 2012 The bipolarity of Supernova 1987A can be understood through its very early light curve from the CTIO 0.4 m telescope and IUE FES and following speckle observations of the “Mystery Spot”. These indicate a beam/jet of light/particles, with initial collimation factors >104 and velocities >0.95 c, involving up to 10−5 M⊙ interacting with circumstellar ...John Middleditch, Alberto J. Castro-Tirado +1 morewiley +1 more sourceConstraining Lorentz Invariance Violation Using the Crab Pulsar Emission Observed up to TeV Energies by MAGIC [PDF]
, 2017 Spontaneous breaking of Lorentz symmetry at energies on the order of the Planck energy or lower is predicted by many quantum gravity theories, implying non-trivial dispersion relations for the photon in vacuum.M. L. Ahnen, S. Ansoldi, L. A. Antonelli, C. Arcaro, A. Babi'c, B. Banerjee, P. Bangale, U. D. Almeida, J. Barrio, J. Gonz'alez, W. Bednarek, E. Bernardini, A. Berti, W. Bhattacharyya, B. Biasuzzi, A. Biland, O. Blanch, S. Bonnefoy, G. Bonnoli, R. Carosi, A. Carosi, A. Chatterjee, S. M. Colak, P. Colin, E. Colombo, J. Contreras, J. Cortina, S. Covino, P. Cumani, P. D. Vela, F. Dazzi, A. Angelis, B. Lotto, E. Wilhelmi, F. D. Pierro, M. Doert, A. Domínguez, D. Prester, D. Dorner, M. Doro, S. Einecke, D. Glawion, D. Elsaesser, M. Engelkemeier, V. Ramazani, A. Fern'andez-Barral, D. Fidalgo, M. V. Fonseca, L. Font, C. Fruck, D. Galindo, R. L'opez, M. Garczarczyk, D. Garrido, M. Gaug, P. Giammaria, N. Godinovi'c, D. Góra, D. Guberman, D. Hadasch, A. Hahn, T. Hassan, M. Hayashida, J. Herrera, J. Hose, D. Hrupec, T. Inada, K. Ishio, Y. Konno, H. Kubo, J. Kushida, D. Kuvevzdi'c, D. Lelas, E. Lindfors, S. Lombardi, F. Longo, M. L'opez, C. Maggio, P. Majumdar, M. Makariev, G. Maneva, M. Manganaro, K. Mannheim, L. Maraschi, M. Mariotti, M. Mart'inez, D. Mazin, U. Menzel, M. Minev, R. Mirzoyan, A. Moralejo, V. Moreno, E. Moretti, V. Neustroev, A. Niedźwiecki, M. N. Rosillo, K. Nilsson, D. Ninci, K. Nishijima, K. Noda, L. Nogu'es, S. Paiano, J. Palacio, D. Paneque, R. Paoletti, J. Paredes, G. Pedaletti, Michele Peresano, L. Perri, M. Persic, P. Moroni, E. Prandini, I. Puljak, J. Garcia, I. Reichardt, W. Rhode, M. Rib'o, J. Rico, C. Righi, T. Saito, K. Satalecka, S. Schroeder, T. Schweizer, J. Sitarek, I. vSnidari'c, D. Sobczynska, A. Stamerra, M. Strzys, T. Suri'c, L. Takalo, F. Tavecchio, P. Temnikov, T. Terzi'c, D. Tescaro, M. Teshima, D. Torres, N. Torres-Albà, A. Treves, G. Vanzo, M. Acosta, I. Vovk, J. Ward, M. Will, D. Z. E. Zurich, CH-8093 Zurich, Switzerland., U. Udine, I. Trieste, I. Udine, Italy., J. Icrr, T. U. O. Tokyo, 277-8582 Chiba, D. Physics, Kyoto University, 606-8502 Kyoto, T. University, 259-1292 Kanagawa, The University of Tokushima, 770-8502 Tokushima, Japan., I. I. F. Astrophysics, I. Rome, U. Padova, Infn, I-35131 Padova, C. Rijeka, 51000 Rijeka, U. O. S. -. Fesb, 21000 Split, U. O. Z. -. Fer, 10000 Zagreb, University of Osijek, 31000 Osijek, Rudjer Boskovic Institute, Croatia., Saha Institute of Nuclear Physics, Hbni, 1. Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India., M. F. Physik, D-80805 Munchen, H Germany, U. Complutense, E. Madrid, Spain., Instituto de Astrof'isica de Canarias, E-38200 La Laguna, U. L. Laguna, D. Astrof'isica, E-38200 La Laguna, Tenerife, University of L'od'z, D. O. Astrophysics, PL-90236 L'od'z, Poland, D. Elektronen-Synchrotron, D. Zeuthen, H. Berlin, Institut fur theoretische Physik, Donald Germany, U. Trieste, I. Trieste, Institut de F'isica d'Altes Energies, T. Z. F. O. Science, Technology, Campus Uab, E-08193 Bellaterra, U. Siena, I. Pisa, I-53100 Siena, Institute for Space Sciences, E. Barcelona, Technische Universitat Dortmund, D. Dortmund, U. Wurzburg, D-97074 Wurzburg, Finnish Magic Consortium Tuorla Observatory, Finnish Magic Consortium Finnish Centre of Astronomy with Eso, U. Turku, 20 Vaisalantie, FI-21500 Piikkio, A. Division, U. Oulu, F. Oulu, Finland., Unitat de F'isica de les Radiacions, D. D. F'isica, CERES-IEEC, U. Barcelona, U. Barcelona, Icc, IEEC-UB, E. Barcelona, Inst. for Nucl. Research, Nucl. Energy, Bulgarian academy of Sciences, BG-1784 Sofia, Bulgaria., U. Pisa, I. Pisa, Icrea +244 moresemanticscholar +1 more sourceFocusing X‐Ray Optics for Astronomy
X-Ray Optics and Instrumentation, Volume 2010, Issue 1, 2010., 2010 Focusing X‐ray telescopes have been the most important factor in X‐ray astronomy’s
ascent to equality with optical and radio astronomy. They are the prime tool for studying
thermal emission from very high temperature regions, non‐thermal synchrotron radiation
from very high energy particles in magnetic fields and inverse Compton scattering of
lower ...Paul Gorenstein, Stephen L. O′Dellwiley +1 more sourceTeraelectronvolt pulsed emission from the Crab pulsar detected by MAGIC [PDF]
, 2015 Aims. We investigate the extension of the very high-energy spectral tail of the Crab Pulsar at energies above 400 GeV.
Methods. We analyzed ~320 h of good-quality Crab data obtained with the MAGIC telescope from February 2007 to April 2014.
Results. We M. C. S. Ansoldi, L. A. Antonelli, P. Antoranz, A. Babić, P. Bangale, U. D. Almeida, J. Barrio, J. Gonz'alez, W. Bednarek, E. Bernardini, B. Biasuzzi, A. Biland, O. Blanch, S. Bonnefoy, G. Bonnoli, F. Borracci, T. Bretz, E. Carmona, A. Carosi, P. Colin, E. Colombo, J. Contreras, J. Cortina, S. Covino, P. D. Vela, F. Dazzi, A. Angelis, G. Caneva, B. Lotto, E. O. Wilhelmi, C. Mendez, F. D. Pierro, D. D. Prester, D. Dorner, M. Doro, S. Einecke, D. Glawion, D. Elsaesser, A. Fern'andez-Barral, D. Fidalgo, M. V. Fonseca, L. Font, K. Frantzen, C. Fruck, D. Galindo, R. L'opez, M. Garczarczyk, D. G. Terrats, M. Gaug, N. Godinovi'c, A. G. Muñoz, S. Gozzini, Y. Hanabata, M. Hayashida, J. Herrera, K. Hirotani, J. Hose, D. Hrupec, G. Hughes, W. Idec, K. Kodani, Y. Konno, H. Kubo, J. Kushida, A. Barbera, D. Lelas, N. Lewankowska, E. Lindfors, S. Lombardi, F. Longo, M. L'opez, R. L'opez-Coto, E. Lorenz, M. Makariev, K. Mallot, G. Maneva, K. Mannheim, L. Maraschi, B. Marcote, M. Mariotti, M. Mart'inez, D. Mazin, U. Menzel, J. Miranda, R. Mirzoyan, A. Moralejo, P. Munar-Adrover, D. Nakajima, V. Neustroev, A. Niedźwiecki, M. N. Rosillo, K. Nilsson, K. Nishijima, K. Noda, R. Orito, A. Overkemping, S. Paiano, J. Palacio, M. Palatiello, D. Paneque, R. Paoletti, J. Paredes, X. Paredes-Fortuny, M. Persic, J. Poutanen, P. Moroni, E. Prandini, I. Puljak, R. Reinthal, W. Rhode, M. Rib'o, J. Rico, J. Garcia, T. Saito, K. Satalecka, V. Scalzotto, V. Scapin, C. Schultz, T. Schweizer, S. Shore, A. Sillanpaa, J. Sitarek, I. Šnidarić, D. Sobczynska, A. Stamerra, T. Steinbring, M. Strzys, L. Takalo, H. Takami, F. Tavecchio, P. Temnikov, T. Terzi'c, D. Tescaro, M. Teshima, J. Thaele, D. Torres, T. Toyama, A. Treves, J. Ward, M. Zanin, E. Zurich, CH-8093 Zurich, Switzerland., U. Udine, I. Trieste, I. Udine, Italy., I. I. F. Astrophysics, I. Rome, U. Siena, I. Pisa, I. Siena, Croatian Magic Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split, U. Zagreb, Croatia., Saha Institute of Nuclear Physics, 1. Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India., M. F. Physik, D-80805 Munchen, H Germany, U. Complutense, E. Madrid, Spain., Instituto de Astrof'isica de Canarias, E-38200 La Laguna, Tenerife, U. L. Laguna, D. Astrof'isica, E-38200 La Laguna, University of L'od'z, PL-90236 Lodz, Poland, D. Elektronen-Synchrotron, D. Zeuthen, Institut de F'isica d'Altes Energies, T. Z. F. O. Science, Technology, Campus Uab, 08193 Bellaterra, U. Wurzburg, D-97074 Wurzburg, U. Padova, Infn, I-35131 Padova, Centro de Investigaciones Energ'eticas, Medioambientales y Tecnol'ogicas, Institute for Space Sciences, E. Barcelona, Technische Universitat Dortmund, D. Dortmund, Unitat de F'isica de les Radiacions, D. D. F'isica, CERES-IEEC, U. Barcelona, E-08193 Bellaterra, U. Barcelona, Icc, IEEC-UB, E. Barcelona, Japanese Magic Consortium, Icrr, T. U. O. Tokyo, D. Physics, H. Center, Kyoto University, T. University, The University of Tokushima, Kek, Japan., Finnish Magic Consortium, T. Observatory, U. Turku, U. Oulu, Finland., Inst. for Nucl. Research, Nucl. Energy, BG-1784 Sofia, Bulgaria., U. Pisa, I. Pisa, Icrea, Now at Centro Brasileiro de Pesquisas F'isicas, R. Sigaud, 150 - Urca, RJ RiodeJaneiro-, 22290-180, Brazil, now at Nasa Goddard Space Flight Center, Greenbelt, MD 20771, Usa, D. O. Astronomy, U. Maryland, College Park, MD 20742, H. Berlin, 15 InstitutfurPhysikNewtonstr., 12489 Berlin Germany, N. C. E. P. F. D. Lausanne, Lausanne, now at Department of PhysicsAstronomy, Uc Riverside, CA 92521, Now at Institut fur Astro- und Teilchenphysik, L. Innsbruck, A. Innsbruck, Austria, also at Japanese Magic Consortium, N. Eso, Turku, also at INAF-Trieste, A. M. C. F. Astrophysics, 1290, Versoix +260 moresemanticscholar +1 more source
