A note on the Little-Tremaine analysis - Estimating the circular speed in the dark halo

Details A note on the Little-Tremaine analysis - Estimating the circular speed in the dark halo A note on the Little-Tremaine analysis - Estimating the circular speed in the dark halo

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.255..680a&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 255, April 15, 1992, p. 680-682.

Statistics

Computation

2

Computational Astrophysics, Galactic Mass, Halos, Milky Way Galaxy, Radial Velocity, Astronomical Models, Gamma Function, Maximum Likelihood Estimates, Natural Satellites

Scientific paper

The Little and Tremaine (LT) analysis in an infinite logarithmic halo
potential Phi(r) = vc squared log r is discussed. The value
of the circular speed vc squared predicted by LT is
considered to be a rescaling of simpler arguements by a factor depending
only on the number of observations.

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