The numerical simulation of astrospheric evolution in different interstellar environments
The interaction between the interstellar medium (ISM) and a stellar wind leads to the formation of an astrosphere. In this study, the evolution of astrospheres is simulated with a two-dimensional spherical hydrodynamic (HD) and magnetohydrodynamic (MHD) model, and a three-dimensional cartesian MHD model.
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The TeV Cosmic-Ray Bump: A Message from the Epsilon Indi or Epsilon Eridani Star? [PDF]
Malkov MA, Moskalenko IV.
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MHD equilibria of astrospheric flows
The hot gas cavities around stars which have a stellar wind are called astrospheres. Between the outer interstellar medium and the stellar wind there forms a contact surface or boundary surface which is called an astropause. In this thesis the geometrical shape of such an astrosphere/astropause region is calculated consistently together with the flow ...
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Imaging magnetically driven astrospheres: a forward modelling approach
An astrosphere is a vast, tailed bubble-like volume around a star, formed through the interaction between the stellar magnetic field, the stellar wind, and the interstellar medium (ISM). Detecting and characterizing astrospheres are essential for constraining stellar wind properties, understanding stellar evolution, and assessing the habitability of ...
Wu, Ziqi +7 more
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Growing Glia: Cultivating Human Stem Cell Models of Gliogenesis in Health and Disease. [PDF]
Lanjewar SN, Sloan SA.
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Application and prospects of high-throughput screening for in vitro neurogenesis. [PDF]
Zhang SY +5 more
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The evolution of the solar wind. [PDF]
Vidotto AA.
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An isogenic blood-brain barrier model comprising brain endothelial cells, astrocytes, and neurons derived from human induced pluripotent stem cells. [PDF]
Canfield SG +7 more
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Human iPSC-Derived Astrocytes: A Powerful Tool to Study Primary Astrocyte Dysfunction in the Pathogenesis of Rare Leukodystrophies. [PDF]
Lanciotti A +4 more
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