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Bulges of spiral galaxies are like the yoke of an egg in the middle
of the spiral disk. They are generally red, like elliptical galaxies, and
also show kinematics that resemble them. Their global parameters,
like their radius and surface brightness, also fall on the relations for
ellipticals.
In the beginning of the 1990's I have started a project, together with
Marc
Balcells (now IAC) to study an optically selected sample of bulges
in detail. Questions were:


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