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The Distribution of the Residual Velocities: A Numerical Method

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Selected Exercises in Galactic Astronomy

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 26))

Abstract

In the preceding exercise we have investigated the distribution of the residual velocities of a group of stars by a graphic method. Now we shall resume this investigation but instead apply a numerical method which essentially represents a translation of the previous one into mathematical terms.

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References

  1. Ogorodnikov, K. F.: 1965, Dynamics of Stellar Systems, Pergamon Press, Oxford.

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  2. Trumpler, R. J. and Weaver, H. F.: 1953, Statistical Astronomy, University of California Press, Berkeley. Reprint: Dover Publications, New York, 1962.

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  3. Mihalas, D., with the collaboration of McRae Routly, P.: 1968, Galactic Astronomy, Freeman and Co., San Francisco.

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  4. Alexander, J. B.: 1958, Monthly Notices Roy. Astron. Soc. 118, 161.

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  5. Charlier, C. V. L.: 1926, The Motion and the Distribution of the Stars, University of California Press, Berkeley.

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© 1971 D. Reidel Publishing Company, Dordrecht, Holland

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Atanasijević, I. (1971). The Distribution of the Residual Velocities: A Numerical Method. In: Selected Exercises in Galactic Astronomy. Astrophysics and Space Science Library, vol 26. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3111-0_5

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  • DOI: https://doi.org/10.1007/978-94-010-3111-0_5

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-3113-4

  • Online ISBN: 978-94-010-3111-0

  • eBook Packages: Springer Book Archive

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