Suspected rotation of an X-ray cluster of galaxies

Details Suspected rotation of an X-ray cluster of galaxies Suspected rotation of an X-ray cluster of galaxies

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984msngr..37...19m&link_type=abstract

ESO Messenger (ISSN 0722-0091), Sept. 1984, p. 19-21.

Physics

1

Dwarf Galaxies, Emission Spectra, Hydrogen Clouds, Stellar Evolution, Stellar Spectra, Wolf-Rayet Stars, Abundance, Red Shift, Spectral Line Width, Stellar Luminosity

Scientific paper

The possible detection of a rotating galaxy cluster is reported. The cluster was observed with the Ariel satellite in the southern hemisphere (03 h, 16 m, -44 degrees) and is tentatively named SC 0316-44. On the basis of measurements of the velocity dispersion of the individual galaxies it could not be shown that the observations were not simply the result of two clusters partially overlapping.

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