The form of galaxy rotation curves, and the presence of neighboring galaxies

Details The form of galaxy rotation curves, and the presence of neighboring galaxies The form of galaxy rotation curves, and the presence of neighboring galaxies

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..264z&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, May 1980, p. 264-268.) Soviet Astronomy Letters, vol. 6, May-June 1980, p. 146-148.

Astronomy and Astrophysics

Astronomy

2

Galactic Rotation, Velocity Distribution, Galactic Structure, Gas Flow, Interstellar Gas, Spatial Distribution, Stellar Motions, Tables (Data)

Scientific paper

Galaxies whose rotation curves pass through a turnover have close
companions more often than do galaxies whose rotation curves end in a
plateau. Neighbor galaxies, even those of low mass, evidently can often
distort the gas-velocity field and the mass distribution in the outer
regions of a given galaxy.

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