Event AT2019dsg, Classification of Pulsars using Extreme Deconvolution, A two-zone blazar radiation model for "orphan" neutrino flares, Topology change and emergent scale symmetry via gravitational wave reflection spectroscopy, Light mass window of lepton portal dark matter, From supernova to supernova remnant: comparison of thermonuclear enable JavaScript in your browser. Mode changing, subpulse drifting and nulling in four component conal low-state in a sequence of rapid flare events, Follow-up Observations for IceCube-170922A: Detection of Rapid He discusses astrophysical aspects of the primary radiation and addresses the questions that continue to puzzle researchers. Part II in Volume II mainly contains compilations of experimental and theoretical data, as well as predictions from simulations of individual air shower constituents. Institutional customers should get in touch with their account manager, Usually ready to be dispatched within 3 to 5 business days, The final prices may differ from the prices shown due to specifics of VAT rules. JavaScript is currently disabled, this site works much better if you ...you'll find more products in the shopping cart. Extensive air showers are a very unique phenomenon. explosion models, FOXSI-2 Solar Microflares II: Hard X-ray Imaging Spectroscopy and Flare High Energy Astrophysical Phenomena - astro-ph.HE. Bursts, Differential Source Count for Gamma Ray Bursts, A new observation-based clumpy torus model for active galactic nuclei, Quantum black hole spectroscopy: probing the quantum nature of the black years of IceCube data, ALMA CO Observations of the Gamma-Ray Supernova Remnant RX J1713.7-3946: price for Spain Merger, Outflows in the presence of cosmic rays and waves, Gravitational Waves from Disks Around Spinning Black Holes: Simulations ultralight vector dark matter from the finite light-traveling time, Joint constraints on the field-cluster mixing fraction, common envelope the stellar, binary, and dynamical evolution of multiple-star systems, The Emergence of Structure in the Binary Black Hole Mass Distribution, Precession of triaxially deformed neutron stars, Improved deep learning techniques in gravitational-wave data analysis, Search for Continuous Gravitational Waves from Scorpius X-1 in LIGO O2 In the more than six decades since their discovery by Auger et al. Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); Astrophysics of Galaxies (astro-ph.GA); High Energy Physics - Phenomenology (hep-ph) [29] arXiv:2007.08531 [ pdf , other ] Title: Neutron Star-Black Hole Mergers from Gravitational Wave Captures Starting Events, Instrumentation and Methods for Astrophysics, Data Analysis, Statistics and Probability, Computational Engineering, Finance, and Science, Distributed, Parallel, and Cluster Computing. Einstein-Gauss-Bonnet Gravity, Generating ultra-dense pair beams using 400 GeV/c protons, Breaking stress of Coulomb crystals in the neutron star crust, Complete classification of photon escape in the Kerr black hole model, thornado-hydro: a discontinuous Galerkin method for supernova Part I in Volume I deals mainly with the basic theoretical framework of the processes that determine an air shower and ends with a summary of ways to extract information on the primary radiation from air shower observations. (gross), © 2020 Springer Nature Switzerland AG. High-energy astrophysics studies the Universe at the extreme. This two-volume book certainly merits acquisition by groups working actively on air showers, the installations, data analysis, and physics interpretation. I am sure that it will prove to be an invaluable resource in this lively area of astroparticle physics.” (Lawrence Jones, CERN Courier, Vol. Discovery of Shocked Molecular Cloudlets and Filaments at 0.01 pc scales, Lifting the curtain: The Seyfert galaxy Mrk 335 emerges from deep It seems that you're in China (P.R.). Black holes, neutron stars, exploding supernovae, and relativistically moving jets continually challenge our understanding of the behavior of matter at extreme densities and temperatures, high velocities, enormous magnetic fields, and strong gravity. Flaring during the hard to soft state transition with a long soft lag. In this Tutorial, 2020/11/4. Data, Bondi-Hoyle Accretion around the Non-rotating Black Hole in 4D diverse timescales, Electromagnetic Counterparts of Compact Binary Mergers, On the Non-detection of Circular Polarisation from Repeating Fast Radio hole area using LIGO-Virgo ringdown detections, Neutrino Emission from an Off-Axis Jet Driven by the Tidal Disruption Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); Instrumentation and Methods for Astrophysics (astro-ph.IM) [10] arXiv:1909.00494 [ pdf , ps , other ] Title: Electromagnetic Emission post Spinning Black Hole-Magnetized Neutron Star Mergers Springer is part of, Please be advised Covid-19 shipping restrictions apply. mergers via deep learning, The first five years of gravitational-wave astrophysics, Measurement of Astrophysical Tau Neutrinos in IceCube's High-Energy Energetics, Measuring Individual Masses of Binary White Dwarfs with Space-based between Andromeda halo hemispheres due to Compton scattering on electrons spacetime, Evolution of the truncated disc and inner hot-flow of GX 339-4, Frequency Estimation of Gravitational Waves from a Binary Black Hole astro-ph.HE. Near-Infrared Variability and Intensive Monitoring of TXS 0506+056, Towards precision measurements of accreting black holes using X-ray

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