Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234..825r&link_type=abstract
Astrophysical Journal, Part 1, vol. 234, Dec. 15, 1979, p. 825-828. Research supported by the Research Corp.
Astronomy and Astrophysics
Astrophysics
41
Astronomical Photometry, Elliptical Galaxies, Galactic Structure, Luminous Intensity, Brightness, Galactic Clusters, Histograms
Scientific paper
The surface brightness-axial ratio relation is investigated in a homogeneous sample of 68 elliptical galaxies in five clusters. The observed correlations favor oblate models over prolate ones in the absence of a correlation between equatorial surface brightness and intrinsic axial ratio. If such a correlation exists, the test is inconclusive. An additional three tests are conducted, one of which is independent of any such correlation. That test accepts both models.
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