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Thermonuclear burst oscillations

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Thermonuclear explosions of rapidly rotating white dwarfs - I. Deflagrations

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Thermonuclear explosions of rapidly rotating white dwarfs - II. Detonations

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Thermonuclear X-ray bursts from the 401 Hertz accreting pulsar IGR J17498-2921: indication of burning in confined regions

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Thin accretion discs around millisecond X-ray pulsars

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Thin accretion disks around neutron and quark stars

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Thin Disk Theory with a Non-Zero Torque Boundary Condition and Comparisons with Simulations

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Three Dimensional MHD Simulation of Circumbinary Accretion Disks: Disk Structures and Angular Momentum Transport

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Three Dimensional Simulations of Vertical Magnetic Flux in the Immediate Vicinity of Black Holes

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Three Millisecond Pulsars in FERMI LAT Unassociated Bright Sources

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Three Regions of Excessive Flux of PeV Cosmic Rays

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Three years of Fermi GBM Earth Occultation Monitoring: Observations of Hard X-ray/Soft Gamma-Ray Sources

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Three Years of Fermi LAT Flare Advocate Activity

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
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Three years Swift-BAT Survey of AGN: reconciling theory and observations?

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Three-dimensional Hydrodynamic Core-Collapse Supernova Simulations for an $11.2 M_{\odot}$ Star with Spectral Neutrino Transport

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Three-dimensional hydrodynamic simulations of the combustion of a neutron star into a quark star

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Three-Dimensional Relativistic Magnetohydrodynamic Simulations of Current-Driven Instability. II. Relaxation of Pulsar Wind Nebula

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Three-Dimensional Simulations of MHD Turbulence Behind Relativistic Shock Waves and Their Implications for GRBs

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Three-dimensional Two-Layer Outer Gap Model: Fermi Energy Dependent Light Curves of the Vela Pulsar

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Three-dimensional Two-Layer Outer Gap Model: the Third Peak of Vela Pulsar

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