Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...287l..21f&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 287, no. 2, p. L21-L24
Astronomy and Astrophysics
Astrophysics
40
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.
Fux Roger
Martinet Louis
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