Results 111 to 120 of about 711 (153)
MHD-shock structures of astrospheres: λ Cephei -like astrospheres [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 The interpretation of recent observations of bow shocks around O-stars and the creation of corresponding models require a detailed understanding of the associated (magneto-)hydrodynamic structures.
K Scherer, L R Baalmann, H Fichtner
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3D MHD astrospheres: applications to IRC-10414 and Betelgeuse [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 A significative fraction of all massive stars in the Milky Way move supersonically through their local interstellar medium (ISM), producing bow shock nebulae by wind-ISM interaction.
D M-A Meyer, A Mignone, K Scherer
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Magnetic Reconnection at Planetary Bodies and Astrospheres
Space Science ReviewsMagnetic reconnection is a fundamental mechanism for the transport of mass and energy in planetary magnetospheres and astrospheres. While the process of reconnection is itself ubiquitous across a multitude of systems, the techniques used for its analysis
D J Gershman, S A Fuselier, M Swisdak
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Lyman-α observations of astrospheres [PDF]
ASTRA Proceedings, 2014 Charge-exchange reactions between outflowing stellar wind protons and interstellar neutral hydrogen atoms entering a stellar astrosphere produce a region of piled-up-decelerated neutral hydrogen called the hydrogen wall.
Jeffrey L Linsky, B E Wood
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On the Diversity of M-star Astrospheres and the Role of Galactic Cosmic Rays Within [PDF]
Astrophysical Journal Letters, 2020 With upcoming missions such as the James Webb Space Telescope, the European Extremely Large Telescope, and the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, we soon will be on the verge of detecting and characterizing Earth-like ...
Konstantin Herbst +2 more
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