The rotation of spiral galaxies

Details The rotation of spiral galaxies The rotation of spiral galaxies

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983sci...220.1339r&link_type=abstract

Science (ISSN 0036-8075), vol. 220, June 24, 1983, p. 1339-1344.

Physics

66

Galactic Rotation, Spiral Galaxies, Angular Velocity, Dark Matter, Histories, Line Spectra, Luminosity, Mass Distribution

Scientific paper

There is accumulating evidence that as much as 90 percent of the mass of the universe is nonluminous and is clumped, halo-like, around individual galaxies. The gravitational force of this dark matter is presumed to be responsible for the high rotational velocities of stars and gas in the disks of spiral galaxies. At present, the form of the dark matter is unknown. Possible candidates span a range in mass of 1070, from non-zero-mass neutrinos to massive black holes.

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