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Shock mechanism of formation of shell-like structures in elliptical galaxies

✍ Scribed by B. I. Gnatyk; V. A. Krol'

Publisher
Springer
Year
1988
Tongue
English
Weight
818 KB
Volume
27
Category
Article
ISSN
0571-7256

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## Abstract The most evident features of colour‐magnitude diagrams of galaxies are the red sequence of quiescent galaxies, extending up to the brightest elliptical galaxies, and the blue cloud of star‐forming galaxies, which is truncated at a luminosity __L__ ∼ __L__~\*~. The truncation of the blue