New redshifts of bright galaxies. II

Details New redshifts of bright galaxies. II New redshifts of bright galaxies. II

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976aj.....81..219d&link_type=abstract

Astronomical Journal, vol. 81, Apr. 1976, p. 219-221. Research supported by the McDonald Observatory and University of Texas

Astronomy and Astrophysics

Astronomy

7

Astronomical Spectroscopy, Galactic Radiation, Red Shift, Spiral Galaxies, Emission Spectra, Galactic Nuclei, Line Spectra, Tables (Data)

Scientific paper

Results are presented for measurements of the redshifts of 14 galaxies, using spectrograms obtained with a low-dispersion B spectrograph at the prime focus of a 205-cm reflector. The galaxies include the largest and brightest galaxy in the Cetus III cloud complex, the brightest member of a group that is part of the Cetus II cloud, a late-type spiral in the N584 group, a late-type spiral in the Virgo III cloud, and a group or chain of five galaxies with bright emission lines in their nuclei. The derived values are found to have a mean error of the order of 50 km/s; no significant systematic differences with previously published values are observed.

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