Statistics – Computation
Scientific paper
Oct 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...321l.113k&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 321, Oct. 15, 1987, p. L113-L115. Research supporte
Statistics
Computation
16
Galactic Mass, Gravitational Lenses, Light Curve, Mass Distribution, Computational Astrophysics, Error Analysis
Scientific paper
Tyson and colleagues deduced bounds on the mass distribution in galaxies, from the (unobserved) distortion of background galaxy images by the gravitational field of foreground galaxies. The authors have checked how critical is their assumption that the background galaxies are at an infinite distance. When the distance distribution of the foreground and background galaxies is taken into account, the upper bounds on the rotation velocities are increased (quite considerably) above those published by Tyson and colleagues in 1984.
Kovner Israel
Milgrom Mordehai
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