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Elliptical galaxies are spheroidal stellar systems with smooth
luminosity profiles which contain old, metal rich stars. They have a
large range in sizes. Usually, rotation is unimportant in ellipticals,
unlike for spirals. They often contain low density, very hot gas that
emits X-rays. The properties of this hot gas, and also the stellar
dynamics, suggest that also in ellipticals most of the mass is in dark
matter.
Subsections
Tom Theuns
平成19年2月7日