Theoretical considerations on the rotation curves of galactic halos

Details Theoretical considerations on the rotation curves of galactic halos Theoretical considerations on the rotation curves of galactic halos

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...157..293m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 157, no. 2, March 1986, p. 293-300.

Astronomy and Astrophysics

Astrophysics

10

Galactic Rotation, Galactic Structure, Halos, Interstellar Matter, Neutrinos

Scientific paper

The influence of the visible matter of the galaxy on the galactic halo is examined in the two limiting configurations of a classical isothermal sphere and a fully degenerate configuration. The authors infer the masses of the particles composing the galactic halos. The possible role of dwarf spheroidal galaxies in probing the structure of the galactic halos at large galactic distance is considered.

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