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Stream Modelling in Angle-Frequency Space

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Part of the book series: Springer Theses ((Springer Theses))

Abstract

The formation of tidal streams reflects the underlying Galactic potential, such that the resulting structures may be used to constrain the potential. One way of using streams to constrain the Galactic potential is to assume that a stream delineates an orbit. This assumption was discussed in Chap. 5, and the results indicate that an improvement over orbit-fitting is required, which accounts for the stream-orbit misalignment.

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Notes

  1. 1.

    Note that, as discussed in Evans (1993), the logarithmic potential produces negative densities for \(q<1/\sqrt{2}\) or \(q>1.08\). Therefore, for a realistic application, we would want to restrict the parameters to ensure we only explore physical models.

  2. 2.

    A logarithmic potential does not tend to an asymptotic limit at large R or z, so technically every orbit in a logarithmic potential is bound. However, in practice, orbits that reach very large R and z take an extremely long time to integrate. Therefore, we consider all orbits which stray more than \(200\,\mathrm{{kpc}}\) from the Galactic centre to be ‘unbound’.

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Correspondence to Jason Sanders .

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© 2015 Springer International Publishing Switzerland

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Sanders, J. (2015). Stream Modelling in Angle-Frequency Space. In: Dynamics of the Milky Way. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-18772-3_6

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