Mass-to-luminosity ratio in binary galaxies

Details Mass-to-luminosity ratio in binary galaxies Mass-to-luminosity ratio in binary galaxies

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.149..141d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 149, no. 1, Nov. 1988, p. 141-147.

Astronomy and Astrophysics

Astrophysics

7

Galactic Radiation, Mass To Light Ratios, Spiral Galaxies, Data Sampling, Frequency Distribution, Monte Carlo Method, Statistical Analysis

Scientific paper

The authors have compared the observed distribution of the quantity log (Vz2rP) for a sample of 233 pairs of galaxies with Monte-Carlo simulations. They have derived an average mass-to-luminosity ratio M/LB = 18±11. The result is consistent with a linear increase of the mass with radius at least until distances of about 30 kpc.

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