Rotation curves for three galaxies - NGC 3077, UGC 5688, UGC 5247

Details Rotation curves for three galaxies - NGC 3077, UGC 5688, UGC 5247 Rotation curves for three galaxies - NGC 3077, UGC 5688, UGC 5247

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..811m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Nov. 1985, p. 811-815) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Nov.-Dec

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Galactic Rotation, H Alpha Line, Light Curve, Astrometry, Galactic Nuclei, Mass To Light Ratios, Spectrum Analysis

Scientific paper

The rotation curves of three galaxies near M81 are determined on the
basis of spectrograms obtained at 550-750 nm and dispersion 5 nm/mm at
the prime focus of the 6-m telescope of the Special Astrophysical
Observatory of the USSR Academy of Sciences during 1982. The data and
results are presented in graphs and a table and briefly characterized.

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