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Elliptical galaxies under perturbation
Astrophysics and Space Science, 1986Three experiments on the initially slightly flattened spheroids (e = 0.45) have been made. The first one is run without perturbation and the others with perturbation. The results have shown that the spheroid without perturbation will evolve to nearly sphere and the other two will almost keep the originally projected shape after perturbation and ...
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On the shape of elliptical galaxies
Journal of Astrophysics and Astronomy, 1983We propose a test for the existence of prolate elliptical galaxies based on the properties of the photometric parameters introduced in the Cordoba surface photometry.
J. L. Sérsic, V. M. Arreguine
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Origin of the Structure Difference Between Elliptical Galaxies and Dwarf Elliptical Galaxies
1999According to the observations of nearby elliptical galaxies, there is a clear distinction in structural and chemical quantities between dwarf ellipticals and normal ellipticals in spite of their morphological similarity. The central concentration of dwarf ellipticals is relatively low and their luminosity profiles are best fitted by an exponential ...
Masao Mori +2 more
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Ellipticity and twisting of isophotes in elliptical galaxies
1979The study of the ellipticity profiles in a sample of elliptical galaxies and the analysis of previous results makes it possible to establish a classification scheme in five classes as follows: increasing ellipticity, decreasing, with maximum, with minimum and constant.
BERTOLA, FRANCESCO, GALLETTA, GIUSEPPE
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Dynamics of early type galaxies. I. The rotation curve of the elliptical galaxy NGC 4697
, 1975F. Bertola, M. Capaccioli
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A unified scenario for the origin of spiral and elliptical galaxy structural scaling laws
Astronomy and Astrophysics, 2021Ismael Ferrero +2 more
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Morphology of interacting elliptical galaxy pairs
Astrophysics and Space Science, 1989Rainer Madejsky
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