The adapted solar wind system as cause for a momentum transfer to the Sun and its consequences for the orbital motions of Keplerian objects

DOI10.1007/BF00627204zbMath0813.70008OpenAlexW1968163377MaRDI QIDQ684460

Hans J. Fahr, Klaus Scherer

Publication date: 16 September 1993

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00627204

zbMATH Keywords

accelerationperturbation analysisperihelionsecular changeswind-driving star

Mathematics Subject Classification ID

Two-body problems (70F05) Celestial mechanics (70F15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (1)

On the motion of wind-driving stars relative to the ambient interstellar medium

Uses Software

• SOLAR

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