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Mixed-Morphology Supernova Remnants in X-rays: Isothermal Plasma in HB21 and Probable Oxygen-Rich Ejecta in CTB 1

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Mock Catalogs for UHECR Studies

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Model analysis of the very high energy detections of the starburst galaxies M82 and NGC 253

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Model of collimated jets with high energy particles

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Model of extended emission of short Gamma-ray Bursts

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Modeling and Maximum Likelihood Fitting of Gamma-Ray and Radio Light Curves of Millisecond Pulsars Detected with Fermi

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Modeling Flows Around Merging Black Hole Binaries

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Modeling Gamma-Ray Burst X-Ray Flares within the Internal Shock Model

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Modeling High-energy and Very-high-energy gamma-rays from the Terzan 5 Cluster

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Modeling high-energy cosmic ray induced terrestrial muon flux: A lookup table

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Modeling high-energy light curves of the PSR B1259-63/LS 2883 binary based on 3-D SPH simulations

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Modeling High-Velocity QSO Absorbers with Photoionized MHD Disk-Winds

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Modeling Light Curves of the Phase-Aligned Gamma-ray Millisecond Pulsar Subclass

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Modeling magnetar outbursts: Flux enhancements and the connection with short bursts and glitches

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Modeling Magnetic Field Amplification in Nonlinear Diffusive Shock Acceleration

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Modeling of Gamma-ray Millisecond Pulsar Light Curves Revealed by Fermi-LAT

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Modeling of Gamma-Ray Pulsar Light Curves with Force-Free Magnetic Field

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Modeling of Photoionized Plasmas

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Modeling of the Interaction of GRB Prompt Emission with the Circumburst Medium

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Modeling pulsar time noise with long term power law decay modulated by short term oscillations of the magnetic fields of neutron stars

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