Rotation of the inner regions of the spiral galaxies NGC 4357, 4814, and 5371

Details Rotation of the inner regions of the spiral galaxies NGC 4357, 4814, and 5371 Rotation of the inner regions of the spiral galaxies NGC 4357, 4814, and 5371

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..455z&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, June 1987, p. 455-463. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astrophysics

4

Galactic Nuclei, Galactic Rotation, Spiral Galaxies, Astronomical Spectroscopy, Mass Ratios

Scientific paper

Rotation curves for the inner regions of NGC 4357, 4814, and 5371 were obtained from spectral observations with the 6-m telescope of the Special Astrophysical Observatory of the USSR Academy of Sciences. The bulge-to-disk mass ratios appear to be very different for the galaxies; and the contribution of the dark halo to the integral inner-part mass appears to be insignificant for all the galaxies.

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