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Effect of Galactic Rotation on Radial Velocities and Proper Motion. Part II

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Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
We express the geometrical and algebraic aspects of the problem of galactic rotation on the motion of the stars represented by fig. (2). We verify the equations involving third order terms of the orbits of the stars. That means taking into account higher order terms in our analysis, namely up to O(r/R0)3. These terms allow a generalization and high precision for the results. We acquired a higher order Taylor’s expansion for V as denoted in fig. (2). U‘, V‘ are the linear components of the velocity of the group of stars S. After some lengthy expansions and reductions, we obtained the formulae for U‘, V‘. Consequently [...], η, ζ the linear components of S corresponding to the two proper motion equalities in galactic longitude and latitude and radial velocity Δρ. Expansions are performed up to the third order in (r/R0).
Rocznik
Strony
261--268
Opis fizyczny
Bibliogr. 5 poz.
Twórcy
autor
  • Astronomy and Space Science Dept. Faculty of Sciences Cairo University, Giza, Egypt
  • Theoretical Physics Dept. National Research Center Dokki, Giza, Egypt
Bibliografia
  • [1] Smart, W. M.: Stellar Kinematics, Ch. 8, Longmans, 1968.
  • [2] Roy, A. E.: Orbital Motion, Fourth Edition, IOP Publishing Ltd., Bristol and Philadelphia, 2005.
  • [3] Smart, W. M.: Spherical Astronomy, Cambridge University Press, fifth Edition, 1965.
  • [4] Binney, J and Termaine, S.: Galactic Dynamics, Princeton University Press, 1987.
  • [5] Stewart, C. A.: Advanced Calculus, Methuen, 1951.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-f5eca14e-07b1-4365-8ffb-583dbf0a838f
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