The disc scale length of the Galaxy

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Galactic Structure, Hydrodynamics, Length, Milky Way Galaxy, Solar Neighborhood, Stellar Systems, Approximation, Drift, Kinematics, Populations, Scale Height, Velocity Distribution

Scientific paper

Analytical approximations valid for a cold and vertically self-gravitating stellar disc are substituted for the velocity dispersion gradients occurring in the asymmetric drift Jeans equation. The resulting equation is then solved at a fixed radius to get the self-consistent exponential scale length hR of the given stellar population as a function of its local kinematical parameters. Application to old disc kinematical data in the solar neighborhood leads to a galactic disc scale length of 2.5+0.8-0.6 kpc if a radially constant scale height (hz) is assumed. However, as suggested by Kent et al. (1991), we argue for an outward increasing hz gradient of 30 pc/kpc increases hR to 3.1 kpc. Such short scale lengths do not suggest a small positive gradient of Toomre's Q parameter in the solar neighborhood.

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