Two broad morphological types characterize most galaxies:
elliptical and spiral forms. The remaining small percentage of
galaxies that cannot be characterized in this way are generally
relegated to the irregular class. The earliest classification schemes
that have had a continuing influence on modern systems were
independently developed by Lundmark
[90] and Hubble
[52]. Discussions
of this early history of galaxy classifications:
[14,
26,
49]. Modern
reviews of the existing classification schemes:
[30,
158
(L5),
195,
199].
The Hubble-Sandage-de Vaucouleurs Classification
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