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Theories of the solar cycle : a critical view

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Theory and Models of Colliding Stellar Winds

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Theory of magnetic reconnection in solar and astrophysical plasmas

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Theory of Solar Meridional Circulation at High Latitudes

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Thermal desorption characteristics of CO, O2 and CO2 on non-porous water, crystalline water and silicate surfaces at sub-monolayer and multilayer coverages

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Thermal fine structure and magnetic fields in the solar atmosphere: spicules and fibrils

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Thermal fluctuations and nanoscale effects in the nucleation of carbonaceous dust grains

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Thermal infrared properties of classical and type II Cepheids Diffraction limited 10 microns imaging with VLT/VISIR

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Thermal instability in ionized plasma

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Thermal instability with the effect of cosmic-ray diffusion

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Thermal Response of A Solar-like Atmosphere to An Electron Beam from A Hot Jupiter: A Numerical Experiment

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Thermalisation and hard X-ray bremsstrahlung efficiency of self-interacting solar flare fast electrons

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Thermally Pulsing Asymptotic Giant Branch Star Models and Globular Cluster Planetary Nebulae I: The Model

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Thermohaline instability and rotation-induced mixing II- Yields of 3He for low- and intermediate-mass stars

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Thermohaline instability and rotation-induced mixing. I - Low- and intermediate-mass solar metallicity stars up to the end of the AGB

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Thermohaline instability and rotation-induced mixing. III - Grid of stellar models and asymptotic asteroseismic quantities from the pre-main sequence up to the AGB for low- and intermediate-mass stars at various metallicities

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Thermohaline Mixing and its Role in the Evolution of Carbon and Nitrogen Abundances in Globular Cluster Red Giants: The Test Case of Messier 3

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Thermohaline mixing and the photospheric composition of low-mass giant stars

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Thermohaline mixing in evolved low-mass stars

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Thermohaline Mixing: Does It Really Govern the Atmospheric Chemical Composition of Low-Mass Red Giants?

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