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    • Keywords


      Stellar systems: dynamics; galaxies: interactions

    • Abstract


      Hernquist’s (1990) mass model for spherical galaxies and bulges described by the deVaucouleur’s profile gives analytical expressions for the density profile and the potential. These have been used to derive a simple and exact analytical expression for the gravitational potential energy of a pair of interpene-trating spherical galaxies represented by this model. The results are compared with those for polytropic and Plummer models of galaxis.

    • Author Affiliations


      K. S. V. S. Narasimhan1 K. S. Sastry1 2 Saleh Mohammed Alladin1

      1. Centre for Astronomy and Astrophysics, Inter University, Ganeshkhind, Pune - 411007, India
      2. Department of Astronomy, Osmania University, Hyderabad - 500007
    • Dates

  • Journal of Astrophysics and Astronomy | News

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      Posted on January 27, 2016

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      Posted on July 25, 2019

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