Disky ellipticals in the Hubble sequence

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

In the present study we investigate the continuity of physical properties between disky ellipticals and S0 galaxies in terms of their D/B ratios and other relevant bulge and disk parameters. We find a smooth transition between both types of galaxies and conclude that, like S0 galaxies, disky ellipticals must have formed in conditions where gas dissipation played a very important role.

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