Elliptical galaxies are one of the three main types of galaxies, the other two being spiral and irregular galaxies. They are named "elliptical" because of their oval or elliptical shape when viewed from above. Elliptical galaxies are composed mainly of older, low-mass stars with little interstellar gas and dust. They are classified according to their shape, ranging from nearly spherical (E0) to highly elongated (E7).
Elliptical galaxies are thought to form through the merger of smaller galaxies and the subsequent disruption of their internal structure. The lack of ongoing star formation and the presence of old stars suggest that elliptical galaxies formed early in the history of the universe. They may also result from the exhaustion of gas and dust in spiral galaxies, leading to the cessation of star formation and the eventual transformation into an elliptical galaxy.
When studying elliptical galaxies, it is important to focus on the following key points:
By mastering these concepts, you will gain a comprehensive understanding of elliptical galaxies and their significance in the study of galaxy formation and evolution.
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