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Missing Matter in the Vicinity of the Sun
Published online by Cambridge University Press: 12 April 2016
Abstract
The combined Poisson-Boltzman equation for the gravitational potential is solved numerically for a detailed Galaxy model. The main result - obtained by comparing the calculated densities with observations of F dwarfs and K giants - is that about half of the mass density in the vicinity of the Sun has not yet been observed.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 78: Astronomy with Schmidt-type telescopes , 1984 , pp. 241 - 246
- Copyright
- Copyright © Reidel 1984