Binary galaxies and massive halos

Details Binary galaxies and massive halos Binary galaxies and massive halos

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976comap...6..127t&link_type=abstract

Comments on Modern Physics, Part C - Comments on Astrophysics, vol. 6, Oct. 1976, p. 127-132.

Astronomy and Astrophysics

Astrophysics

2

Galactic Structure, Galaxies, Halos, Galactic Radiation, Galactic Rotation, Mass Ratios, Radial Velocity, Spiral Galaxies, Velocity Distribution

Scientific paper

Determinations of the mass-to-light ratios (M/L) of binary galaxies are examined in some detail to investigate why the binary-galaxy method of M/L determination gives results smaller than those given by the rotation-curve and velocity-dispersion methods. Selection biases inherent to the binary-galaxy method are identified, and results are summarized for a recent attempt at determining the M/L ratios of 156 binary galaxy systems. These results are shown to be in rough agreement with other external measures of galactic masses and are considered as supporting the massive-halo hypothesis. Several qualitative effects of dynamical friction in binary galaxy systems whose components possess massive halos are discussed.

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